List of Publications
Kohji Tomisaka
ORCID ID: 0000-0003-2726-0892
ResearcherID: E-6508-2013

August 29, 2024
pdf: http://th.nao.ac.jp/MEMBER/tomisaka/Papers/list/list.pdf
Refereed Journal[115]. Instability and Evolution of Shocked Clouds Formed by Orthogonal Collisions Between
Magnetized Filamentary Molecular Clouds, 2024, Aug., Astrophysical Journal in press,
R. Kashiwagi, K. Iwasaki, and K. Tomisaka (doi:10.3847/1538-4357/ad7389; arXiv:2408.08863)[114]. An Extremely Young Protostellar Core, MMS 1 / OMC-3: Episodic Mass Accretion
History Traced by the Micro SiO Jet, 2024, Mar., Astrophysical Journal, 964, 48(14pp),
by S. Takahashi, M.N. Machida, M. Omura, D. Johnstone, N. Harada, K. Tomisaka,
K. Saigo, P.T.P. Ho, L.A. Zapata, S. Mairs, G.J.Herczeg, Y. Liu, K.Taniguchi, and
A. Sato (doi:10.3847/1538-4357/ad2268; arXiv:2401.13204)[113]. Dust Polarization of Prestellar and Protostellar Sources in OMC-3, 2024, Mar., Astrophysical Journal, 963, 104(33pp), by Y. Liu, S. Takahashi, M.N. Machida, K. Tomisaka,
J.M.Girart, K. Nakanishi, P.T.P. Ho, and A. Sato (doi:10.3847/1538-4357/ad182d; arXiv:2312.13573)[112]. Filamentary Network and Magnetic Field Structures Revealed with BISTRO in theHigh-Mass Star-Forming Region NGC2264 – Global Properties and Local MagnetoGravitational Conﬁgurations, 2024, Feb., Astrophysical Journal, 962, 136(34pp), by
J.-W. Wang, P.M. Koch, S.D. Clarke, et al.(BISTRO Team) (doi:10.3847/1538-4357/ad165b;
arXiv:2401.12728)[111]. Simulation of Head-on Collisions between Filamentary Molecular Clouds Threaded bya Lateral Magnetic Field and Subsequent Evolution, 2023, Aug., Astrophysical Journal,
954, 129(18pp), by R. Kashiwagi, K. Iwasaki, and K. Tomisaka (doi:10.3847/15384357/ace7bd; arXiv:2307.07698)[110]. The JCMT BISTRO Survey: Studying the Complex Magnetic Field of L43, 2023, July,
Astrophysical Journal, 952, 29(18pp), J. Karoly, D. Ward-Thompson, K. Pattle, etal.(BISTRO Team) (doi:10.3847/1538-4357/acd6f2; arXiv:2305.11306)[109]. First BISTRO Observations of the Dark Cloud Taurus L1495A-B10: the Role of theMagnetic Field in 4 the Earliest Stages of Low-mass Star Formation, 2023, April,
Astrophysical Journal, 946, 62(12pp), by D. Ward-Thompson, et al.(BISTRO Team)(doi:10.3847/1538-4357/acbea4; arXiv:2302.12058)[108]. JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with
NGC 6334, 2023, Feb., Astrophysical Journal, 944, 139(21pp), by M. Tahani, et al.(BISTROTeam) (doi:10.3847/1538-4357/acac81; arXiv:2212.10884)
1[107]. Twisted Magnetic Field on Star Formation Processes in L1521 F Revealed by Submillimeter Dual Band Polarimetry Using JCMT, 2023, Jan., Publications Astronomical Society Japan, 75, 120, S. Fukaya,, H. Shinnaga, R.S. Furuya, K. Tomisaka, M.N. Machida,
and N. Harada (doi:10.1093/pasj/psac094; arXiv:2211.08988)[106]. The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament, 2022,
Dec., Astrophysical Journal, 941, 122(21pp), by Tao-Chung Ching, et al. (BISTROTeam) (doi:10.3847/1538-4357/ac9dfb; arXiv:2212.01981)[105]. The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-Filament Structure,
Monoceros R2, 2022, Dec., Astrophysical Journal, 941, 51(19pp), by J. Hwang, J. Kim,
K. Pattle, C.W. Lee, P.M. Koch, D. Johnstone, K. Tomisaka, et al. (BISTRO Team)(doi:10.3847/1538-4357/ac99e0; arXiv:2210.05937)[104]. Mushroom-instability-driven Magnetic Reconnections in Collisionless Relativistic Jets,
2022, Mar., Astrophysical Journal, 928, 62(10pp), by T. Kawashima, S. Ishiguro, T. Moritaka,
R. Horiuchi, and K. Tomisaka (doi:10.3847/1538-4357/ac5591; arXiv:2202.09706)[103]. B-ﬁelds in Star-Forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main, 2022, Feb., Astrophysical Journal, 926, 163(13pp),
by W. Kwon, et al. (BISTRO Team) (doi:10.3847/1538-4357/ac4bbe; arXiv:2201.05059)[102]. The JCMT BISTRO Survey: Evidence for Pinched Magnetic Fields in Quiescent Filaments of NGC 1333, 2021, Nov., Astrophysical Journal (Letters), 923, L9(12pp),
by Y. Doi, K. Tomisaka, T. Hasegawa, et al. (BISTRO Team) (doi:10.3847/20418213/ac3cc1; arXiv:2111.12230)[101]. The JCMT BISTRO Survey: An 850/450 µm Polarization Study of NGC 2071IR
in Orion B, 2021, June, Astrophysical Journal, 918, 85(17pp), by A-Ran Lyo et al.
(BISTRO Team) (doi:10.3847/1538-4357/ac0ce9; arXiv:2109.133543)[100]. Super-Fast Rotation in the OMC 2/FIR 6b Jet, 2021, July, Astrophysical Journal, 916,23(9pp), Y. Matsushita, S. Takahashi, S. Ishii, K. Tomisaka, P. Ho, J. Carpenter, and
M.N. Machida (doi:10.3847/1538-4357/ac069f; arXiv:2107.12002)[99]. Revealing the Diverse Magnetic Field Morphologies in Taurus Dense Cores with Sensitive
Sub-millimeter Polarimetry, 2021, May, Astrophysical Journal (Letters), 912, L27(15pp),
by E. Chakali, et al. (BISTRO Team) (doi:10.3847/2041-8213/abeb1c; arXiv:2103.02219)[98]. Magnetohydrostatic Equilibrium Structure and Mass of Polytropic Filamentary CloudThreaded by Lateral Magnetic Field, 2021, April, Astrophysical Journal 911, 106(15pp),
by R. Kashiwagi and K. Tomisaka (doi:10.3847/1538-4357/abea7a; arXiv:2103.02846)[97]. Dust Polarized Emission Observations of NGC 6334; BISTRO Reveals the Details of
the Complex but Organized Magnetic Field Structure of the High-Mass Star-Forming
Hub-Filament Network, 2021, Mar., Astronomy and Astrophysics, 647, A78(29pp), by
D. Arzoumanian et al. (BISTRO Team) (doi:10.1051/0004-6361/202038624; arXiv:2012.13060)
2

[96]. Observations of Magnetic Fields Surrounding LkH α 101 Taken by the BISTRO Survey
with JCMT-POL-2, 2020, Dec., Astrophysical Journal, 908, 10(20pp) by Nguyen Bich Ngoc,
et al. (BISTRO Team) (doi:10.3847/1538-4357/abd0fc; arXiv:2012.04297)[95]. Distortion of Magnetic Fields in the Dense Core SL 42 (CrA-E) in the Corona Australis Molecular Cloud Complex, 2020, Sept., Astrophysical Journal, 900, 20(13pp), by
R. Kandori, M. Tamura, M. Saito, K. Tomisaka, T. Matsumoto, R.Tazaki, T. Nagata,
N. Kusakabe, Y. Nakajima, J. Kwon, T. Nagayama, and K. Tatematsu (doi:10.3847/15384357/abaab3; arXiv:2007.15436)[94]. The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in
NGC 1333, 2020, Aug., Astrophysical Journal, 899, 28(33pp), by Y. Doi et al. (BISTROTeam) (doi:10.3847/1538-4357/aba1e2; arXiv:2007.00176); Erratum Astrophysical Journal, 911, 72 (2021) (doi:10.3847/1538-4357/abf2b3)[93]. Disk Structure around the Class I Protostar L1489 IRS Revealed by ALMA: A Warpeddisk System, 2020, April, Astrophysical Journal, 893, 51(21pp), by J. Sai, N. Ohashi,
K. Saigo, T. Matsumoto, Y. Aso, S. Takakuwa, Y. Aikawa, I. Kurose, H.-W. Yen, K. Tomisaka,
K. Tomida, and M.N. Machida, (doi:10.3847/1538-4357/ab8065; arXiv:2003.07067)[92]. Distortion of Magnetic Fields in BHR 71, 2020, Feb., Astrophysical Journal, 892, 128(7pp),
by R. Kandori, M. Tamura, M. Saito, K. Tomisaka, T. Matsumoto, R. Tazaki, T. Nagata,
N. Kusakabe, Y. Nakajima, J. Kwon, T. Nagayama, and K. Tatematsu (doi:10.3847/15384357/ab7b68; arXiv:2002.12512)[91]. Distortion of Magnetic Fields in Barnard 335, 2020, Mar., Astrophysical Journal, 891,
55(13pp), by R. Kandori, M. Saito, M. Tamura, K. Tomisaka, T. Matsumoto, R. Tazaki,
T. Nagata, N. Kusakabe, Y. Nakajima, J. Kwon, T. Nagayama, and K. Tatematsu (doi:10.3847/15384357/ab6f07)[90]. Distortion of Magnetic Fields in Barnard 68, 2020, Feb., Publications Astronomical Society Japan, 72, 8(17pp), by R. Kandori, M. Tamura, M. Saito, K. Tomisaka, T. Matsumoto,N. Kusakabe, J. Kwon, T. Nagayama, T. Nagata, R. Tazaki, and K. Tatematsu (doi:10.1093/pasj/psz12
arXiv:1910.09121)[89]. Distortion of Magnetic Fields in the Dense Core CB81 (L1774, Pipe 42) in the Pipe
Nebula, 2020, Feb., Astrophysical Journal, 890, 14(16pp), by R. Kandori, K. Tomisaka,
M. Saito, M. Tamura, T. Matsumoto, R. Tazaki, T. Nagata, N. Kusakabe, Y. Nakajima,
J. Kwon, T. Nagayama, and K. Tatematsu (doi:10.3847/1538-4357/ab67c5; arXiv:1912.10029)[88]. Distortion of Magnetic Fields in a Starless Core. VI. Application of Flux Freezing Model
and Core Formation of FeSt 1 - 457, 2020, Jan., Astrophysical Journal, 888, 120(18pp),
by R. Kandori, K. Tomisaka, M. Saito, M. Tamura, T. Matsumoto, R. Tazaki, T. Nagata,
N. Kusakabe, Y. Nakajima, J. Kwon, T. Nagayama, and K. Tatematsu (doi:10.3847/15384357/ab6081; arXiv:1912.02935)3

[87]. Fragmentation of Filamentary Cloud Permeated by Perpendicular Magnetic Field II.
Dependence on the Initial Density Proﬁle, 2019, Aug., Astrophysical Journal, 881,
97(13pp), by T. Hanawa, T. Kudoh, and K. Tomisaka (doi:10.3847/1538-4357/ab2d26;
arXiv:1907.03384v1)[86]. The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-Forming Region,
2019, June, Astrophysical Journal, 877, 88(17pp), by S. Coude et al. (BISTRO Team)(doi:10.3847/1538-4357/ab1b23; arXiv:1904.07221)[85]. The JCMT BISTRO Survey: The Magnetic Field In The Starless Core ρ Ophiuchus C,
2019, May, Astrophysical Journal, 877, 43(17pp), by J.-H. Liu, et al. (BISTRO Team)(doi:10.3847/1538-4357/ab0958; arXiv:1902.07734)[84]. JCMT BISTRO survey: Magnetic Fields within the Hub-Filament Structure in IC 5146,
2019, May, Astrophysical Journal, 876, 42(19pp), by J.-W. Wang, et al. (BISTRO Team)(doi:10.3847/1538-4357/ab13a2; arXiv:1812.05818)[83]. ALMA High Angular Resolution Polarization Study; An Extremely Young Class 0
Source, OMC-3/MMS 6, 2019, Feb., Astrophysical Journal, 872, 70(15pp), by S. Takahashi,
M.N. Machida, K. Tomisaka, P.T.P. Ho, E.B. Fomalont, and K. Nakanishi (doi:10.3847/15384357/aaf6ed; arXiv:1812.03189)[82]. A Very Compact Extremely High Velocity Flow toward MMS 5 / OMC-3 Revealedwith ALMA, 2019, Feb., Astrophysical Journal, 871, 221(12pp), by Y. Matsushita,
S. Takahashi, M.N. Machida, and K. Tomisaka (doi:10.3847/1538-4357/aaf1b6; arXiv:1811.08060)[81]. Distortion of Magnetic Fields in a Starless Core V: Near-infrared and Submillimeter Polarization in FeSt 1 - 457, 2018, Oct., Astrophysical Journal, 868, 94(6pp) by R. Kandori,
M. Tamura, K. Tomisaka, T. Matsumoto, N. Kusakabe, Y. Nakajima, J. Kwon, T. Nagayama,
T. Nagata, and K. Tatematsu (doi:10.3847/1538-4357/aae888; arXiv:1810.05996)[80]. Distortion of Magnetic Fields in a Starless Core IV: Magnetic Field Scaling on Density
and Mass-to-ﬂux Ratio Distribution in FeSt 1 - 457, 2018, Aug., Astrophysical Journal, 865, 121(10pp), by R. Kandori, K. Tomisaka, M. Tamura, M. Saito, N. Kusakabe,
Y. Nakajima, J. Kwon, T. Nagayama, T. Nagata, and K. Tatematsu (doi:10.3847/15384357/aadb3f; arXiv:1808.05327)[79]. Magnetic Fields towards Ophiuchus-B Derived from SCUBA-2 Polarization Measurements, 2018, July, Astrophysical Journal, 861, 65(13pp), by A. Soam, et al. (BISTROTeam) (doi:10.3847/1538-4357/aac4a6; arXiv:1805.06131)[78]. A First Look at BISTRO Observations of the ρ Oph-A Core, 2018, Mar., Astrophysical Journal, 859, 4(22pp), by J. Kwon, et al. (BISTRO Team) (doi:10.3847/15384357/aabd82; arXiv:1804.09313)[77]. Distortion of Magnetic Fields in a Starless Core III: Polarization-Extinction Relationship in FeSt 1 - 457, 2018, April, Astrophysical Journal, 857, 100(7pp), by R. Kandori,4

M. Tamura, N. Kusakabe, Y. Nakajima, J. Kwon, T. Nagayama, T. Nagata, K. Tomisaka,and K. Tatematsu (doi:10.3847/1538-4357/aab962; arXiv:1803.08196v1)[76]. Circumnuclear Multi-phase Gas in Circinus Galaxy I: Non-LTE calculations of CO lines,
2018, Jan. Astrophysical Journal, 852, 88(11pp), by K. Wada, R. Fukushige, T. Izumi,
and K. Tomisaka (doi:10.3847/1538-4357/aa9e53; arXiv:1711.10117)[75]. ALMA Observations of SMM11 Reveal an Extremely Young Protostar in Serpens Main
Cluster, 2017, Nov., Astrophysical Journal, 850, L2(6pp), by Y. Aso, N. Ohashi, Y. Aikawa,
M. N. Machida, K. Saigo, M. Saito, S. Takakuwa, K. Tomida, K. Tomisaka, H.-W. Yen,
and J. P. Williams (doi:10.3847/2041-8213/aa9701; arXiv:1710.10787)[74]. ALMA Observations of the Protostar L1527 IRS: Probing Detailed Structures of the Disk
and the Envelope, 2017, Nov., Astrophysical Journal, 849, 56(15pp), Y. Aso, N. Ohashi,
Y. Aikawa, M.N. Machida, K. Saigo, M. Saito, S. Takakuwa, K.Tomida, K. Tomisaka,and H.-W. Yen (doi:10.3847/1538-4357/aa8264; arXiv:1707.08697)[73]. Distortion of Magnetic Fields in a Starless Core II: 3D Magnetic Field Structure of FeSt
1 - 457, 2017, Oct., Astrophysical Journal, 848, 110(7pp) by R. Kandori, M. Tamura,
K. Tomisaka, Y. Nakajima, N. Kusakabe, J. Kwon, T. Nagayama, T. Nagata, and K. Tatematsu(doi:10.3847/1538-4357/aa8d18; arXiv:1709.04544)[72]. Fragmentation of Filamentary Cloud Permeated by Perpendicular Magnetic Field, 2017,
Oct., Astrophysical Journal, 848, 2(12pp), T. Hanawa, T Kudoh, and K. Tomisaka(doi:10.3847/1538-4357/aa8b6d; arXiv:1709.05149)[71]. Distortion of Magnetic Fields in a Starless Core: Near-Infrared Polarimetry of FeSt
1 - 457, 2017, Aug., Astrophysical Journal, 845, 32(10pp), by R. Kandori, M. Tamura,
N. Kusakabe, Y. Nakajima, J. Kwon, T. Nagayama, T. Nagata, and K. Tomisaka (doi:10.3847/15384357/aa7d58; arXiv:1707.00720)[70]. The Evidence of Radio Polarization Induced by the Radiative Grain Alignment and
Self-Scattering of Dust Grains in a Protoplanetary Disk, 2017, July, Astrophysical Journal (Letters), 844, L5(5pp), by A. Kataoka, T. Tsukagoshi, A. Pohl, T. Muto, H. Nagai,
I.W. Stephens, K. Tomisaka, and M. Momose (doi:10.3847/2041-8213/aa7e33; arXiv:1707.01612)[69]. First Results from BISTRO: A SCUBA-2 Polarimeter Survey of the Gould Belt, 2017,
June, Astrophysical Journal, 842, 66(10pp), by D.Ward-Thompson et al. (BISTROTeam) (doi:10.3847/1538-4357/aa70a0; arXiv:1704.08552)[68]. ALMA Observations of the Transition from Infall Motion to Keplerian Rotation aroundthe Late-phase Protostar TMC-1A, 2015, Oct., Astrophysical Journal, 812, 27(20pp),
by Y. Aso, N. Ohashi, K. Saigo, S. Koyamatsu, Y. Aikawa, M. Hayashi, M.N. Machida,
M. Saito, S. Takakuwa, K. Tomida, K. Tomisaka, and H.-W. Yen (doi:10.1088/0004637X/812/1/27; arXiv:1508.07013) Erratum ApJ, 836, 148(1pp) (2015) (doi:10.3847/15384357/836/1/148)5

[67]. Polarization Structure of Filamentary Clouds, 2015, July, Astrophysical Journal, 807,
47(10pp), by K. Tomisaka (doi:10.1088/0004-637X/807/1/47; arXiv:1505.02895) Erratum, Astrophysical J., 920, 161(1pp) (2021) (doi:10.3847/1538-4357/ac295a)[66]. Structure and Stability of Filamentary Clouds Supported by Lateral Magnetic Field,
2015, March, Astrophysical Journal, 801, 11(11pp), by T. Hanawa, and K. Tomisaka(doi:10.1088/0004-637X/801/1/11; arXiv:1501.07734)[65]. Formation of a Keplerian Disk in the Infalling Envelope around L1527 IRS: Rransformation from Infalling Motions to Kepler Motions, 2014, Dec., Astrophysical Journal, 796,
131(11pp), by N. Ohashi, K. Saigo, Y. Aso, Y. Aikawa, S. Koyamatsu, M.N. Machida,
M. Saito, S.Z. Takahashi, S. Takakuwa, K. Tomida, K. Tomisaka, and H.-W. Yen, (doi:10.1088/0004637X/796/2/131; arXiv:1410.0172)[64]. ALMA Observations of Infalling Flows toward the Keplerian Disk around the Class I
Protostar L1489 IRS, 2014, Sept., Astrophysical Journal, 793, 1(20pp), by H.-W. Yen,
S. Takakuwa, N. Ohashi, Y. Aikawa, Y. Aso, S. Koyamatsu, M.N. Machida, K. Saigo, M. Saito,
K. Tomida, and K. Tomisaka, (doi:10.1088/0004-637X/793/1/1; arXiv:1407.2699)[63]. Structure and Mass of Filamentary Isothermal Cloud Threaded by Lateral Magnetic
Field, 2014, April, Astrophysical Journal, 785, 24(12pp), by K. Tomisaka (doi:10.1088/0004637X/785/1/24; arXiv:1402.3033) Erratum, ApJ, 861, 155(1pp) (2018) (doi:10.3847/15384357/aacea6)[62]. Radiation Magnetohydrodynamic Simulations of Protostellar Collapse: Protostellar Core
Formation, 2013, Jan., Astrophysical Journal, 763, 6(29pp), by K. Tomida, K. Tomisaka,
T. Matsumoto, Y. Hori, S. Okuzumi, M.N. Machida, and K. Saigo (doi:10.1088/0004637X/763/1/6; arXiv:1206.3567)[61]. Exploring Magnetic Field Structure in Star-Forming Cores with Polarization of Thermal Dust Emission, 2012, Nov., Astrophysical Journal. 761, 40(21pp), by A. Kataoka,
M.N. Machida, and K. Tomisaka (doi:10.1088/0004-637X/761/1/40; arXiv:1210.7637)[60]. Chemistry in the First Hydrostatic Core Stage by Adapting Three-Dimensional Radiation Hydrodynamic Simulations, 2012, Oct., Astrophysical Journal, 758, 86(20pp), by
K. Furuya, Y. Aikawa, K. Tomida, T. Matsumoto, K. Saigo, K. Tomisaka, F. Hersant,and V. Wakelam (doi:doi:10.1088/0004-637X/758/2/86; arXiv:1207.6693)[59]. Magnetic Field in the Isolated Massive Dense Clump IRAS 20126+4104, 2012, May, Astrophysical Journal (Letters), 750, L29(5pp), by H. Shinnaga, G. Novak, J.E. Vaillancourt,
M.N. Machida, A. Kataoka, K. Tomisaka, J. Davidson, T.G. Phillips, C.D. Dowell, L. Leeuw,
and M. Houde (doi:10.1088/2041-8205/750/2/L29; arXiv:1203.3211)[58]. Origin of Multiple Nuclei in Ultraluminous Infrared Galaxies, 2012, Feb., AstrophysicalJournal, 746, 26(11pp), by H. Matsui, T.R. Saitoh, J. Makino, K. Wada, K. Tomisaka,
E. Kokubo, H. Daisaka, T. Okamoto, and N. Yoshida (doi:10.1088/0004-637X/746/1/26)

6

[57]. Observational Identiﬁcation of First Cores: Non-LTE Radiative Transfer Simulation,
2011, Oct., Publications Astronomical Society Japan, 63, 1151–1164, by K. Tomisaka,and K. Tomida (doi:10.1093/pasj/63.5.1151; arXiv:1104.2438)[56]. Spectrum Energy Distribution and Submillimeter Image of a Rotating First Core, 2011,
Feb., Astrophysical Journal, 728, 78(10pp), by K. Saigo, and K. Tomisaka (doi:10.1088/0004637X/728/2/78)[55]. Origin of Molecular Outﬂow Determined from Thermal Dust Polarization, 2011, Feb.,
Publicaltions Astronomical Society Japan, 63, 147–158, by K. Tomisaka (doi:10.1093/pasj/63.1.147;
arXiv:1011.0125) Erratum, June PASJ 63, 715–715 (2011) (doi:10.1093/pasj/63.3.715)[54]. Exposed Long-lifetime First-core; A New Model of the First Core Based on Radiation
Hydrodynamics, 2010, Dec., Astrophysical Journal Letters, 725, L239–L244, K. Tomida,
M.N. Machida, K. Saigo, K. Tomisaka, and T. Matsumoto (doi:10.1088/2041-8205/725/2/L239;
arXiv:1011.4951) Erratum, ApJL, 732, L18(1pp) (2011) (doi:10.1088/2041-8205/732/1/L18)[53]. Radiation Magnetohydrodynamics Simulation of Proto-Stellar Collapse: Two-Component
Molecular Outﬂow, 2010, May, Astrophysical Journal, 714, L58–L63, K. Tomida, K. Tomisaka,
T. Matsumoto, K. Ohsuga, M.N. Machida, and K. Saigo (doi:10.1088/2041-8205/714/1/L58;
arXiv:1001.4796)[52]. Emission from a Young Protostellar Object I. Signatures of Young Embedded Outﬂows,
2009, Sept., Astrophysical Journal, 703, 1141–1158, by M. Yamada, M.N. Machida, S.i. Inutsuka, and K. Tomisaka (doi:10.1088/0004-637X/703/1/1141; arXiv:0908.1874)[51]. Formation of Galactic Center Magnetic Loops, 2009, June, Publications Astronomical
Society Japan, 61, 411–420, by M. Machida, R. Matsumoto, S. Nozawa, K. Takahashi,
Y. Fukui, N. Kudo, and K. Tomisaka (doi:10.1093/pasj/61.3.411; arXiv:0812.3711)[50]. Toward First-Principle Simulations of Galaxy Formation: II. Shock-Induced Starburst at
a Collision Interface During the First Encounter of Interacting Galaxies, 2009, June, Publications Astronomical Society Japan, 61, 481–486, by T.R. Saitoh, H. Daisaka, E. Kokubo,
J. Makino, T. Okamoto, K. Tomisaka, K. Wada, and N. Yoshida (doi:10.1093/pasj/61.3.481;
arXiv:0805.0167)[49]. How Was the Mushroom-Shaped GW 123.4-1.5 Formed in the Galactic Disk?, 2008, August, Astrophysical Journal, 682, 434–444, by C.H. Baek, T. Kudoh, and K. Tomisaka(doi:10.1086/589556; arXiv:0801.3186)[48]. Toward First-Principle Simulations of Galaxy Formation: I. How Should We Choose
Star Formation Criteria in High-Resolution Simulations of Disk Galaxies?, 2008, August, Publ. Astron. Soc. Japan, 60, 667–681, by T.R. Saitoh, H. Daisaka, E. Kokubo,
J. Makino, T. Okamoto, K. Tomisaka, K. Wada, and N. Yoshida (doi:10.1093/pasj/60.4.667;
arXiv:0802.0961)

7[47]. Formation Scenario for Wide and Close Binary Systems, 2008, April, Astrophysical Journal, 677, 327–347, by M.N. Machida, K. Tomisaka, T. Matsumoto, and S. Inutsuka(doi:10.1086/529133; arXiv:0709.2739)[46]. Evolution of First Cores and Formation of Stellar Cores in Rotating Molecular Cloud
Cores, 2008, Feb., Astrophysical Journal, 674, 997–1014, by K. Saigo, K. Tomisaka,
and T. Matsumoto (doi:10.1086/523888)[45]. HCN to HCO+ Millimeter Line Diagnostics of AGN Molecular Torus. I: Radiative Transfer Modeling, 2007, Dec., Astrophysical Journal, 671, 73–84, by M. Yamada, K. Wada,
and K. Tomisaka (doi:10.1086/522332; arXiv:0708.1045)[44]. Evolution of Rotating Molecular Cloud Core with Oblique Magnetic Field, 2006, July.,
Astrophysical Journal, 645, 1227–1245, by M.N. Machida, T. Matsumoto, T. Hanawa,
and K. Tomisaka (doi:10.1086/504423; arXiv:astro-ph/0602034)[43]. Evolution of First Core in Rotating Molecular Cores, 2006, July, Astrophysical Journal,
645, 381–394, by K. Saigo, and K. Tomisaka (doi:10.1086/504028)[42]. Long-Term Evolution of Supernova Remnants in Magnetized Interstellar Medium, 2006,
April, Astrophysical Journal, 641, 905–918. by H. Hanayama, and K. Tomisaka(doi:10.1086/500527; arXiv:astro-ph/0507421)[41]. Alignment of Outﬂows with Magnetic Fields in Cloud Cores, 2006, Feb., AstrophysicalJournal (Letters), 637, L105–L108, by T. Matsumoto, T. Nakazato, and K. Tomisaka(doi:10.1086/500646; arXiv:astro-ph/0512581)[40]. Collapse and Fragmentation of Rotating Magnetized Clouds. II. Binary Formation andFragmentation of First Cores, 2005, Sept., Monthly Notices Royal Astronical Society,362, 382–402, M.N. Machida, T. Matsumoto, T. Hanawa, and K. Tomisaka (doi:10.1111/j.13652966.2005.09327.x; arXiv:astro-ph/0506440)[39]. Collapse and Fragmentation of Rotating Magnetized Clouds. I. Spin and Mass-toFlux Ratio Relation, 2005, Sept., Monthly Notices Royal Astronical Society, 362, 369–
381, M.N. Machida, T. Matsumoto, K. Tomisaka, and T. Hanawa (doi:10.1111/j.13652966.2005.09297.x; arXiv:astro-ph/0506439)[38]. Low-Mass Star Formation, Triggered by Supernova in Primordial Clouds, 2005, March,
Astrophysical Journal, 622, 39–57, by M.N. Machida, K. Tomisaka, F. Nakamura, and
M. Y. Fujimoto (doi:10.1086/428030; arXiv:astro-ph/0412282)[37]. Molecular Gas Structure around the AGN with the Nuclear Starbursts: Observational
Visualization by 3-D Non-LTE Calculations of CO Lines, 2005, Jan., Astrophysical Journal, 619, 93 –104, by K. Wada, and K. Tomisaka (doi:10.1086/426377; arXiv:astroph/0410254)

8

[36]. Directions of Outﬂow, Disk, Magnetic Field, and Rotation of YSOs in Collapsing Molecular Cloud Cores, 2004, Nov., Astrophysical Journal, 616, 266 – 282, by T. Matsumoto,and K. Tomisaka (doi:10.1086/424897; arXiv:astro-ph/0408086)[35]. First MHD Simulation of Collapse and Fragmentation of Magnetized Molecular Cloud
Cores, 2004, Feb., Monthly Notices Royal Astronical Society, 348, L1 – L5, by M.N. Machida,
K. Tomisaka, and T. Matsumoto (doi:10.1111/j.1365-2966.2004.07402.x; arXiv:astroph/0311339)[34]. Collapse of Rotating Magnetized Molecular Cloud Core and Mass Outﬂows, 2002, Aug.,
Astrophysical Journal, 575, 306 – 326, by K. Tomisaka (doi:10.1086/341133; arXiv:astroph/0105527)[33]. The Evolution of the Angular Momentum Distribution during Star Formation, 2000,
Jan., Astrophysical Journal (Letters), 528, L41 – L44, by K. Tomisaka (doi:10.1086/312417;
arXiv:astro-ph/9911166)[32]. Gravitational Collapse of Spherical Isothermal Clouds, 1999, Oct., Publications Astronomical Society Japan, 51, 637 – 651, by S. Ogino, K. Tomisaka, and F. Nakamura(doi:10.1093/pasj/51.5.637)[31]. Gravitational Collapse of Isothermal Magnetized Clouds: Universality of Self-similar
Collapse, 1999, Jan., Astrophysical Journal, 510, 274–290, by F. Nakamura, T. Matsumoto,
T. Hanawa, and K. Tomisaka (doi:10.1086/306553)[30]. Superbubbles in Magnetized Interstellar Media: Blowout or Conﬁnement?, 1998, Aug.,
Monthly Notices Royal Astronomical Society, 298, 797 – 810, by K. Tomisaka (doi:10.1046/j.13658711.1998.01654.x; arXiv:astro-ph/9804029)[29]. Collapse-Driven Outﬂow in Star-Forming Molecular Cores, 1998, Aug., AstrophysicalJournal (Letters), 502, L163 – L167, by K. Tomisaka (doi:10.1086/311504; arXiv:astroph/9806085)[28]. Recent X-ray Observations of SN 1986J with ASCA and ROSAT, 1998, Jan, Astrophysical Journal, 493, 431 – 439, by J.C. Houck, J.N. Bregman, R.A. Chevalier, andK. Tomisaka (doi:10.1086/305098; arXiv:astro-ph/9703193)[27]. Accretion in Gravitationally Contracting Clouds, 1996, Oct., Publications Astronomical
Society Japan, 48, L97 – L101, by K.Tomisaka (doi:10.1093/pasj/48.5.L97; arXiv:astroph/9610001)[26]. Collapse and Fragmentation of Magnetized Cylindrical Clouds: Simulation with Nested
Grid Scheme, 1996, Oct., Publications Astronomical Society Japan, 48, 701 – 717, by
K. Tomisaka (doi:10.1093/pasj/48.5.701; arXiv:astro-ph/9411040)[25]. Collapse and Fragmentation of Magnetized Cylindrical Clouds, 1995, Jan., AstrophysicalJournal, 438, 226 – 243 by K. Tomisaka (doi:10.1086/175067; arXiv:astro-ph/9306028)

9[24]. High Resolution X-ray Imaging of the Starburst Galaxy M82, 1995, Jan., AstrophysicalJournal, 439, 155 – 162, by J.N. Bregman, E. Shulman, and K. Tomisaka (doi:10.1086/175160)[23]. X-ray Emission from the Starburst Galaxy IC 342, 1993, Oct., Astrophysical Journal(Letters), 415, L79 – L82, by J.N. Bregman, C.V. Cox, and K. Tomisaka (doi:10.1086/187037)[22]. Extended Hot Gas Halos around Starburst Galaxies, 1993, Aug., Publications of Astronomical Society of Japan, 45, 513 – 528, by K. Tomisaka, and J.N. Bregman (arXiv:astroph/9209002; ads:1993PASJ...45..513T)[21]. 12 CO (J = 1 − 0) Mapping of the Merging Galaxy NGC 3310, 1993, Aug., Astronomical
Journal, 106, 466 – 472, by T. Kikutomo, Y. Taniguchi, M. Suzuki, and K. Tomisaka(doi:10.1086/116655)[20]. The Evolution of a Magnetized Superbubble, 1992, Sept., Publications of Astronomical
Society of Japan, 44, 177 – 191, by K. Tomisaka (ads:1992PASJ...44..177T)[19]. Two-Component Gravitating Systems and Red-Giant Like Structure, 1992, Feb., Astrophysical Journal, 385, 445 – 459, by M.Y. Fujimoto, and K. Tomisaka. (doi:10.1086/170954)[18]. The Equilibria and Evolutions of Magnetized, Rotating, Isothermal Clouds V. The Efectof Toroidal Field, 1991, July, Astrophysical Journal, 376, 190 –198, by K. Tomisaka(doi:10.1086/170267)[17]. The Equilibria and Evolutions of Magnetized, Rotating, Isothermal Clouds IV. Quasistatic Evolution, 1990, Oct., Astrophysical Journal, 362, 201 – 214, by K. Tomisaka,
S. Ikeuchi, and T. Nakamura (doi:10.1086/169255)[16]. Blow-out of Superbubble in Galactic Magnetic Field, 1990, Sept., Astrophysical Journal(Letters), 361, L5 – L8 by K. Tomisaka (doi:10.1086/185814)[15]. The Equilibria and Evolutions of Magnetized, Rotating, Isothermal Clouds III. Critical
Mass, 1989, June, Astrophysical Journal, 341, 220 – 237, by K. Tomisaka, S. Ikeuchi,
and T. Nakamura (doi:10.1086/167487) Erratum ApJ, 346, 1061 – 1062 (1989) (doi:10.1086/168090)[14]. The Equilibria and Evolutions of Magnetized, Rotating, Isothermal Clouds II. The Extreme Case: Non-Rotating Clouds, 1988, Dec., Astrophysical Journal, 335, 239 – 262,
by K. Tomisaka, S. Ikeuchi, and T. Nakamura (doi:10.1086/166923)[13]. Starburst Nucleus: Galactic-Scale Bipolar Flow, 1988, July Astrophysical Journal, 330,
695 – 717, by K. Tomisaka and S. Ikeuchi (doi:10.1086/166505)[12]. The Equilibria and Evolutions of Magnetized, Rotating, Isothermal Clouds I. Basic
Equations and Numerical Methods, 1988, March, Astrophysical Journal, 326, 208 – 222,
by K. Tomisaka, S. Ikeuchi, and T. Nakamura (doi:10.1086/166082)[11]. Galactic Shock in Cloud Fluid and Its Gravitational Instability, 1987, Mar., Publications
Astronomical Society Japan, 39, 109 – 131, by K. Tomisaka (ads:1987PASJ...39..109T)
10

[10]. Evolution of a Superbubble Driven by Sequential Supernova Explosions in a PlaneStratiﬁed Gas Distribution, 1986, Nov., Publications Astronomical Society Japan, 38,697 – 715, by K. Tomisaka, and S. Ikeuchi (ads:1986PASJ...38..697T)[9]. A Possible Contribution of Supernova Remnants to the Excess X-ray Emission from the
Galactic Ridge, 1986, Aug., Publications Astronomical Society Japan, 38, 503 – 509, by
K. Koyama, S. Ikeuchi, and K. Tomisaka (ads:1986PASJ...38..503K)[8]. Formation of Giant Molecular Clouds by Coagulation of Small Clouds and Spiral Structure, 1986, March, Publications Astronomical Society Japan, 38, 95 – 110, by K. Tomisaka(ads:1986PASJ...38...95T)[7]. Gravitational Instability of Neutrino-Dominated Pancakes and Galaxy Formation, 1985,
Oct., Publications Astronomical Society Japan, 37, 461 – 480, by K. Tomisaka, andS. Ikeuchi (ads:1985PASJ...37..461T)[6]. Coagulation of Interstellar Clouds in Spiral Gravitational Potential and Formation of
Giant Molecular Clouds, 1984, Nov., Publications Astronomical Society Japan, 36, 457– 476, by K. Tomisaka (ads:1984PASJ...36..457T)[5]. Gravitational Instability of Isothermal Gas Layers: Eﬀect of Curvature and Magnetic
Field, 1983, Aug, Publications Astronomical Society Japan, 35, 187 – 208, by K. Tomisaka,
and S. Ikeuchi (ads:1983PASJ...35..187T)[4]. The Structure and Expansion Law of a Shock Wave in an Expanding Universe, 1983,
Feb., Astrophysical Journal, 265, 583 – 596, by S. Ikeuchi, K. Tomisaka, and J.P. Ostriker(doi:10.1086/160703)[3]. Interaction of Intergalactic-Gas Flow with a Rigid-Body, Spheroidal Galaxy, 1981, Dec.,
Astrophysics and Space Science, 80, 483 – 500, by S. Ikeuchi, and K. Tomisaka (doi:10.1007/BF00652[2]. Sequential Explosions of Supernovae in an OB Association and Formation of a Superbubble, 1981, Aug., Astrophyics and Space Science, 78, 273 – 285, by K. Tomisaka,
A. Habe and S. Ikeuchi (doi:10.1007/BF00648941)[1]. Missing Supernova Remnants, 1980, Nov., Progress of Theoretical Physics, 64, 1587 –
1595, by K. Tomisaka, A. Habe and S. Ikeuchi (doi:10.1143/PTP.64.1587)

11

Volume Editor[4]. Tenmongaku Jiten (Astronomy Dictionary), 2012, (Tokyo: Nippon Hyoronsha ISBN13: 978-4535607385) eds. S. Okamura, M. Iye, S. Inutsuka, K. Koyama, M. Chiba, andK. Tomisaka (in Japanese)[3]. Simyureshon Tenmongaku (Simulation Astronomy), 2007, (Tokyo: Nippon Hyoronsha
ISBN-13: 978-4535607347) eds. K. Tomisaka, T. Hanawa, and J. Makino (in Japanese)[2]. Numerical Astrophysics, 1999, proceedings of the International Conference on Numerical Astrophysics 1998 (NAP98), held at the National Olympic Memorial Youth Center, Tokyo, Japan, March 10-13, 1998 (Dordrecht: Kluwer Academic Publishers, ISBN:0792355660) eds. S.M. Miyama, K. Tomisaka, and T. Hanawa (doi:10.1007/978-94-0114780-4; ads:1999ASSL..240.....M)[1]. Numerical Astrophysics by Ultra-High Speed Computers 1993, National Astronomical
Observatory Reports, edited by S. M. Miyama, and K. Tomisaka

12Proceedings, etc[51]. Structures of Magnetically-Supported Filaments and Their Appearance In the Linear
Polarization, Oct. 2017, in Submm/mm/cm QUESO Workshop 2017 (QUESO2017),
Centimetre-Sub-Millimetre Q&U (and V) European Southern Observatory Workshop,
held 25-27 October, 2017 at ESO, Garching bei München, Germany.
Online at https://www.eso.org/sci/meetings/2017/QUESO2017.html, id.29(doi:10.5281/zenodo.1038105)[50]. Structure and Stability of Filamentary Clouds Supported by Lateral Magnetic Field,
2015, Aug., in IAU General Assembly, Meeting #29, Honolulu, Aug, 2015, by T. Hanawa,
and K. Tomisaka (ads:2015IAUGA..2243208H)[49]. SMA and ALMA Studies of Protoplanetary-Disk Formation around Low-mass Protostars, 2015, Aug. in IAU General Assembly, Meeting #29, Honolulu, Aug., 2015, by
S. Takakuwa, H.-W. Yen, N. Ohashi, T.-L. Chou, Y. Aso, K. Saigo, M. Saito, M.N. Machida,
K. Tomida, Y. Aikawa, K. Tomisaka, S. Koyamatsu, S.Z. Takahashi (ads:2015IAUGA..2230558T)[48]. Structure and Mass of Filamentary Isothermal Cloud Threaded by Lateral Magnetic
Field, 2013, July, in Protostars and Planets VI, Heidelberg, July 15-20, 2013. Poster#1S026 (p.76 of Abstract Book), by K. Tomisaka (ads:2013prpl.conf1S026T)[47]. Molecular Evolution in the First Hydrostatic Core Phase Adapting Three-Dimensional
Radiation Hydrodynamic Simulations, 2013, Oct., in New Trends in Radio Astronomy
in the ALMA Era: The 30th Anniversary of Nobeyama Radio Observatory. Proceedings of a Symposium held in Hakone, Japan 3-8 December 2012, ASP Conference Series, Vol. 476. San Francisco: Astronomical Society of the Paciﬁc, 2013., p.385, by
K. Furuya, Y. Aikawa, K. Tomida, T. Matsumoto, K. Saigo, K. Tomisaka, F. Hersant,and V. Wakelam (ads:2013ASPC..476..385F)[46]. Expected Observations of the Star Formation Process: from Molecular Cloud Core toFirst Hydrostatic Core, 2012, July, in EPoS 2012 The Early Phase of Star Formation- Assembling Pieces of the Missing Paradigm Sunday, 1 July 2012 - Friday, 6 July
2012, Max-Planck-Society Conference Center Ringberg Castle, Tegernsee, Germany, by
K. Tomisaka, A. Kataoka, M.N. Machida, and K. Tomida ∗[45]. Expected Observations of the Star Formation Process: from Molecular Cloud Core toFirst Hydrostatic Core, 2014, in The Labyrinth of Star Formation: A Conference Dedicated to Prof. Anthony Whitworth 18-22 June 2012, Crete, Greece, by K. Tomisaka,
A. Kataoka, M.N. Machida, and K. Tomida, in Astrophysics and Space Science Proceedings, Volume 36 (ISBN 978-3-319-03040-1) (Springer International Publishing; Switzerland), p. 133 (doi:10.1007/978-3-319-03041-8 24; ads:2014ASSP...36..133T)[44]. Hydrodynamical-Chemical Models from Prestellar Cores to Protostellar Cores, The
Molecular Universe, Proceedings of the International Astronomical Union, IAU Symposium, Volume 280, pp. 33–42, by Y. Aikawa, K. Furuya, V. Wakelam, F. Hersant,T. Matsumoto, K. Saigo, K. Tomida, K. Tomisaka, R. Garrod, E. Herbst
13

[43]. Molecular Evolution of A First Core in 3 Dimensional Hydrodynamic Calculations, 2011,
May, The Molecular Universe, Posters from the proceedings of the 280th Symposium of
the International Astronomical Union held in Toledo, Spain, May 30-June 3, 2011, #166,
by K. Furuya, Y. Aikawa, T. Matsumoto, K. Tomida, K. Saigo, K. Tomisaka, F. Hersant,V. Wakelam (ads:2011IAUS..280P.166F)[42]. Shock-induced star cluster formation in colliding galaxies, 2011, Jan., in Proceedingsof IAU Symposium 270, “Computational Star Formation” by T.R. Saitoh, H. Daisaka,
E. Kokubo, J. Makino, T. Okamoto, K. Tomisaka, K. Wada, and N. Yoshida (doi:10.1017/S174392131
arXiv:1101.3708)[41]. Shock-Induced Starburst and Star Cluster Formation in Colliding Galaxies, in “Galaxy
Wars: Stellar Populations and Star Formation in Interacting Galaxies”, proceedings ofa conference held 19-22 July 2009 at East Tennessee State University, Johnson City,
Tennessee, USA. Edited by B. Smith, N. Bastian, S.J.U. Higdon, and J.L. Higdon. San
Francisco: Astronomical Society of the Paciﬁc (Conference Series), 423, p.185 (2010)
by T.R. Saitoh, H. Daisaka, E. Kokubo, J. Makino, T. Oakmoto, K. Tomisaka, K. Wada,
and N. Yoshida (ads:2010ASPC..423..185S)[40]. Three Dimensional Line Transfer Study of Energy Sources in Compact Molecular Gas
in Active Galaxies — AGN/Starburst Connection — presented at ”The Starburst-AGN
Connection Conference”. October 27-31, 2009, Shanghai by M. Yamada, K. Wada andK. Tomisaka (arXiv:arXiv:0811.3541; ads:2009ASPC..408..254Y)[39]. Eﬀect of Magnetic Fields in Star Formation Process, presented at “10th Asian-Paciﬁc
Regional IAU Meeting,” held in August 3–6, 2008, in Yunnan, China, by K.Tomisaka[38]. Eﬀect of Magnetic Field in Star Formation, presented at “TIARA Workshop on Radiative Transfer, Chemistry, and Numerical Simulation”, held in July 7 – 11, 2008 at
National Taiwan University, Taipei by K. Tomisaka∗[37]. Current Advances in the Computational Simulation of the Formation of Low-Mass Stars
in “Protostars and Planets. V” (October 24 – 28, 2005; Waikoloa, Hawaii) edited by
B. Reipurth, D. Jewitt, and K. Keil, U. Arizona Press, Tucson, pp. 99 – 116, 2007 by
R.I. Klein, S. Inutsuka, P. Padoan, and K. Tomisaka (arXiv:arXiv:astro-ph/0603711;
ads:2007prpl.conf...99K)[36]. Fragmentation and Evolution of the First Core, in the 2nd East-Asia Numerical Astrophysics Meeting, held November 1-3, 2006, at Korea Astronomy and Space Science
Institute in Daejeon, Korea, by K. Tomisaka and K. Saigo ∗[35]. Evolution of First Core in Rotating Molecular Cores, in Abstract book of IAU Symposium #237 “Triggered Star Formation in a Turbulent ISM” held 14-18 August, 2006 in
Prague, Czech Republic by K. Saigo, and K. Tomisaka[34]. Contraction of a Magnetized Rotating Cloud, presented at EPoS 2006 “The Early Phaseof Star Formation,” held August 28 – September 1, 2006, in Ringberg Castle, Tegernsee,
Germany by K. Tomisaka. ∗14

[33]. The Evolution of the First Core in Rotating Molecular Core, in Protostars and Planets V, Proceedings of the Conference held October 24 – 28, 2005, in Hilton Waikoloa
Village, Hawai’i. LPI Contribution No. 1286., p. 8624 by K. Saigo, and K. Tomisaka(arXiv:arXiv:astro-ph/0510469; ads:2005prpl.conf.8624S)[32]. Collapse and Fragmentation of Rotating Magnetized Clouds: Parallel Rotators with B// Omega, in Protostars and Planets V, Proceedings of the Conference held October 24– 28, 2005, in Hilton Waikoloa Village, Hawai’i. LPI Contribution No. 1286., p. 8280, by
M.N. Machida, T. Matsumoto, T. Hanawa, and K. Tomisaka. (ads:2005prpl.conf.8280M)[31]. Orientation of Disk and Outﬂows Formed Through Collapse of a Rotating Molecular
Cloud Core with Oblique Magnetic Fields, in Protostars and Planets V, Proceedingsof the Conference held October 24 – 28, 2005, in Hilton Waikoloa Village, Hawai’i.
LPI Contribution No. 1286., p. 8279, by M.N. Machida, T. Matsumoto, T. Hanawa, andK. Tomisaka. (ads:2005prpl.conf.8279M)[30]. Collapse and Fragmentation of a Magnetized Molecular Cloud — 3D Nested Grid MHD
Simulation — in “East Asia Numerical Astrophysics Meeting” (November 30 – December
2, 2004; Mitaka, Japan) by M.N. Machida, T. Matsumoto, K. Tomisaka, and T. Hanawa∗[29]. Alignment of Outﬂow, Magnetic Field, Disk, and Rotation in Protostellar Collapse, in“East Asia Numerical Astrophysics Meeting” (Nov. 30 – Dec. 2, 2004; Mitaka, Japan)
by T. Matsumoto and K. Tomisaka. ∗[28]. How Magnetic Fields Aﬀect the SNR Evolution, in “Diﬀuse Matter in the Galaxy:
Observations Confront Theory,” (Aug. 29 – Sept. 2, 2004; Arecibo, Puerto Rico) by
K. Tomisaka ∗[27]. Role of Magnetic Field in Star Formation Process, in ”The Magnetized Plasma in Galaxy
Evolution,” held in Jagiellonian University, Cracow, Poland, September 27 - October
01, 2004, eds. K.T. Chyzy, R.-J. Dettmar, K. Otmianowska-Mazur, and M. Soida, Jagiellonian University, pp.111 – 116 written by K. Tomisaka, M.N. Machida, T. Matsumoto,and T. Hanawa (ads:2005mpge.conf..111T)[26]. Evolution of the Galactic Cores and Structure of the Molecular Gas Tori, in “The Interplay among Black Holes, Stars and ISM in Galactic Nuclei,” Proceedings IAU Symposium #222, held in Gramado, Brazil, Mar. 1-5, 2004, eds. Th.S. Bergmann, L.C. Ho, and
H.R. Schmitt, Cambridge U. Pr., pp. 401 – 406 (2004) authored by K. Wada, T.R. Saitoh,and K. Tomisaka (doi:10.1017/S174392130400273X; ads:2004IAUS..222..401W)[25]. Numerical Simulations of Collapse and Fragmentation of Magnetized Molecular Cloud
Cores — Formation of Binary Systems, in Proceedings of “Gravitational Collapse: From
Massive Stars to Planets” Dec. 2004, First Astrophysics meeting of the Observatorio Astronomico Nacional (Mexico) held in Ensenada, Baja California, December 8 - 12, 2003,(Eds. G. Garcı́a-Segura, G. Tenorio-Tagle, J. Franco, and H.W. Yorke) Revista Mexicana

15

de Astronomı́a y Astrofı́sica (Serie de Conferencias), 22, pp. 18 – 21 (2004) written by
K. Tomisaka, M.N. Machida, T. Matsumoto, and K. Saigo (ads:2004RMxAC..22...18T)[24]. Binary Star Formation and Mass Outﬂows: MHD Nested Grid Simulation, in “TheEnvironment and Evolution of Double and Multiple Stars,” Aug. 2004, Proceedingsof IAU Colloquium 191, held 3-7 February, 2002 in Merida, Yucatan, Mexico. Edited
by C. Allen and C. Scarfe Revista Mexicana de Astronomı́a y Astrofı́sica (Serie de Conferencias), 21, pp. 168 – 172 (2004) authored by M.N. Machida, K. Tomisaka, andT. Matsumoto (ads:2004RMxAC..21..168M)[23]. Self-gravitational Collapse of a Magnetized Cloud Core: High Resolution Simulations
with Three-dimensional MHD Nested Grid, 2004, in “Proceedings of the 18th International Conference on Numerical Simulation of Plasmas,” (Sept.7–10, 2003, Cape
Cod, U.S.) Computer Physics Communications Journal, 164, 229 – 236, written by
T. Matsumoto, M.N. Machida, K. Tomisaka, and T. Hanawa (doi:10.1016/j.cpc.2004.06.033;
ads:2004CoPhC.164..229M)[22]. Evolution of Supernova Remnants in Magnetized Interstellar Medium, 2003, (Proceedings of International Workshop “How Does the Galaxy Work,” (June 23–27, 2003),
Granada, Spain, written by K.Tomisaka. ∗[21]. Contraction and Fragmentation of Magnetized Rotating Clouds and Formation of Binary Systems, 2004, Astrophysics and Space Science 292, 309–316, 2004 Special Issue:“Magnetic Fields and Star Formation: Theory Versus Observations,” eds. A.I. Gómez
de Castro, M. Heyer, E. Vázquez-Semadeni, R. Rrebolo, M. Tagger and R.E. Pudritz(April 21 - 25, 2003), Madrid, Spain, written by K. Tomisaka, M.N. Machida, andT. Matsumoto. (doi:10.1023/B:ASTR.0000045032.47925.54; ads:2004Ap&SS.292..309T)[20]. Fragmentation of Molecular Clouds and Binary Star Formation, in Star Formation atHigh Angular Resolution, International Astronomical Union. Symposium no. 221,
held 22-25 July, 2003 in Sydney, Australia p.167, by M.N. Machida, K. Tomisaka, andT. Matsumoto (ads:2003IAUS..221P.167M)[19]. Outﬂow from YSO and Angular Momentum Transfer, 2000, Proceedings of the IAU
Simposium on “The Formation of Binary Stars” (April 10-15, 2000) AIP, Potsdam,
Germany, pp. 401 – 405 , written by K. Tomisaka. (arXiv:arXiv:astro-ph/0006329;
ads:2001IAUS..200..401T)[18]. Outﬂows from YSO’s and the Angular Momentum of New-Born Stars, June 2000, Proceedings of 33rd ESLAB Symposium on “Star Formation from the Small to the Large
Scale” (November 2-5, 1999) ESTEC, Noordwijk, The Netherlands, pp. 141 – 148,
written by K. Tomisaka. (ads:2000ESASP.445..141T)[17]. Collapse-Driven Outﬂow in Star-Forming Molecular Cores, 2000, in “Star Formation
1999” (proceedings of a meeting held at Nagoya University, Nagoya, Japan June 21 – 25,1999), edited by T. Nakamoto, pp.197 – 198, written by K. Tomisaka (ads:1999sf99.proc..197T)

16

[16]. Gravitational Contraction of Magnetized Clouds, 1999, in Numerical Astrophysics, eds.
S.M. Miyama, K. Tomisaka, and T. Hanawa, (Kluwer Academic Publishers: Dordrecht),
pp.141 – 150, written by K. Tomisaka (doi:10.1007/978-94-011-4780-4 45; ads:1999ASSL..240..141T)[15]. Fragmentation, contraction, and accretion in magnetized clouds, 1997, Low Mass Star
Formation - from Infall to Outﬂow, Poster proceedings of IAU Symposium No. 182
on Herbig-Haro Objects and the Birth of Low Mass Stars. 20-24 January 1997, Chamonix, France, Edited by F. Malbet and A. Castets, p. 250, written by K.Tomisaka(ads:1997IAUS..182P.250T)[14]. 12 CO (J=1-0) Mapping of the Merging Galaxy NGC 3310, 1994, in “Astronomy with
Millimeter and Submillimeter Wave Interferometry,” IAU Colloquium 140, ASP Conference Series, Vol. 59, eds. M. Ishiguro and J. Welch, p.374, by T. Kikutomo, Y. Taniguchi,
M. Suzuki, and K. Tomisaka. (ads:1994ASPC...59..374K)[13]. X-ray Emission from Starburst Outﬂows, 1994, in “New Horizon of X-ray Astronomy —First Results from ASCA —” eds. F. Makino and T. Ohashi (Universal Academy Pr.:
Tokyo), pp.525 – 526, written by K. Tomisaka. (ads:1994nhxr.conf..525T)[12]. Collapse and Fragmentation of Magnetized Cylindrical Clouds, 1994, presented at 1st
UNAM-Cray Workshop on “Numerical Simulations in Astrophysics” held in Mexico City,
Mexico, July 26-30, 1993, ed. by J. Franco, S. Lizano, L. Aguilar, and E. Daltabuit (Cambridge Univ. Pr.), pp. 336 – 340, written by K. Tomisaka (ads:1994nsa..book..336T)[11]. The Evolution of Superbubble and Supernova Remnant in the Magnetized Interstellar Medium, 1994, presented at 1st UNAM-Cray Workshop on “Numerical Simulationsin Astrophysics” held in Mexico City, Mexico, July 26-30, 1993, ed. by J. Franco,
S. Lizano, L. Aguilar, and E. Daltabuit (Cambridge Univ. Pr.), pp. 184 – 191, written by K. Tomisaka. (ads:1994nsa..book..184T)[10]. Hot Gas Outﬂows from Starburst Galaxies, 1993, Aug., in “Star Formation, Galaxies
and the Interstellar Medium,” (presented at EIPC/ESO Workshop held in Marciana
Mariana, Isola d’Elba, Italy, on June 1-6, 1992), ed. by J. Franco, F. Ferrini, and G.
Tenorio-Tagle (Cambridge Univ. Pr.), pp. 265–267, written by K. Tomisaka, and Joel
N. Bregman[9]. Evolution of a Superbubble in the Magnetized Interstellar Medium, 1993, Aug., in “Star
Formation, Galaxies and the Interstellar Medium,” presented at EIPC/ESO Workshop
held in Marciana Mariana, Isola d’Elba, Italy, on June 1-6, 1992, ed. by J. Franco,
F. Ferrini, and G. Tenorio-Tagle (Cambridge Univ. Pr.), pp.262–264, written by K. Tomisaka(ads:1993sfgi.conf..262T)[8]. Numerical simulations of Galactic Inﬂow Outﬂow Phenomena, 1991, Aug., presented as areview talk at IAU Symposium #144 on “The Interstellar Disk-Halo Interface in Galaxies” held in Leiden, the Netherlands, on June 18-22, 1990, ed. by J.B.G.M. Bloemen(Reidel), pp. 407-416, written by K. Tomisaka (ads:1991IAUS..144..407T)

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[7]. Evolution of Magnetized, Rotating, Isothermal Clouds, 1990, presented at the Second Wyoming Conference on “The Interstellar Medium in External Galaxies” held in
Wyoming, U.S.A. on July 3-7, 1989, ed. by D. Hollenbach (NASA), H.A. Thronson(U.Wyoming), pp.255 – 257, written by K. Tomisaka (ads:1990NASCP3084..255T)[6]. Collective Eﬀects of Supernova Explosions in Starburst Nucleus, 1989, presented at
Yamada Conference XX on “Big Bang, Active Galactic Nuclei and Supernovae,” held inTokyo on March 28-April 1, 1988, ed. by S. Hayakawa and K. Sato (Universal Academic
Press), p.603, written by K. Tomisaka (ads:1989bbag.conf..603T)[5]. Collective Eﬀects of Supernova Explosions in Starburst Nucleus, 1988, March, presented
at IAU Colloquium 101, “The Interaction of Supernova Remnants with the Interstellar Medium,” held in Penticton, Canada on June 8 - 12, 1987, published in Supernova Remnants and the Interstellar Medium, ed. by R. S. Roger and T. L. Landecker(Cambridge University Press), pp.477-480, written by K. Tomisaka, and S. Ikeuchi.
(ads:1988srim.conf..477T)[4]. Formation of Giant Molecular Clouds by Coagulation of Small Molecular Clouds in a
Spiral Gravitational Potential, 1987, Jan. presented at IAU Symposium No. 115 “Star
Forming Regions,” held in Tokyo on Nov. 11 - 15, 1985, published in Proceeding of IAU
Symposium 115 ed. by M. Peimbert and J. Jugaku, (Reidel,Dordrecht), pp.541 – 543
written by K. Tomisaka (ads:1987IAUS..115..541T)[3]. Cycling of the Local Interstellar Matter, 1986, Nov., presented as a review talk at
COSPAR Symposium “UV Space Astronomy: Physical Processes in the Local Interstellar Matter,” held in Toulouse on July 4 and 5, 1986, published in Advances in Space
Research, 6, pp.109 – 118, ed. by C. Gry and W. Wamsteker, written by K. Tomisaka(ads:1986AdSpR...6b.109T)[2]. Structure and Evolution of Superbubbles in the Stratiﬁed Gas Distribution, 1985, published in Theoretical Aspects on Structure, Activity, and Evolution of Galaxies: III,
Proceedings of a Japanese Symposium on Galaxies held at Tokyo Astronomical Observatory, 21-23 January, 1985. Edited by Shinko Aoki, Masanori Iye, and Yuzuru Yoshii.
Japan: Tokyo Astronomical Observatory, University of Tokyo, 1985., p.25 written by
K. Tomisaka (ads:1985tasa.conf...25T)[1]. Coagulation of Interstellar Clouds in Spiral Gravitational Potential and Formation of
Giant Molecular Clouds published in Theoretical Aspects on Structure, Activity, andEvolution of Galaxies: II, Proceedings of a Japanese Symposium on Galaxies held at
Tokyo Astronomical Observatory, 14-16 February, 1984. Edited by Shinko Aoki and
Yuzuru Yoshii. Japan: Tokyo Astronomical Observatory, University of Tokyo, 1984.,
p.79, written by K. Tomisaka (ads:1984tasa.conf...79T)
As of August 29, 2024, I have published 115 refereed papers, and 43 proceeding papers. In
addition, I have edited 5 books.
∗

represents no proceedings.
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