Delta Crucis - Wikipedia
Die Suiderkruis, met Delta Crucis regs.
Spektraaltipe B2 IV
Regte klimming 12h 15m 08.71673s
Deklinasie -58° 44′ 56.1369″
Skynmagnitude (m) 2,79
Absolute magnitude (M) -3,2
Massa (M☉) 8,9 ± 0,1
Radius (R☉) 8
Ligsterkte (L☉) 10 000
Ouderdom (jaar) 18,1 ± 3,2 miljoen
Temperatuur (K) 22 570 ± 1 840
Rotasiespoed (km/s) 210
Veranderlikheid β Cep
CD-58 4466, FK5 455, HD 106490, HIP 59747, HR 4656, SAO 239791.
Delta Crucis (δ Crucis, afgekort as Delta Cru of δ Cru) is ’n ster in die suidelike sterrebeeld Suiderkruis (Crux). Dit het ’n skynbare magnitude van 2,79 en is sowat 345 ligjare van die Son af. Dit is die dofste van die vier helder sterre wat die asterisme Suiderkruis vorm. Delta Crucis het ’n groot massa, hoë temperatuur en vinnige rotasiespoed, en is besig om in ’n reusester te ontwikkel.
Die ster het ’n sterreklassifikasie van B2 IV, en is dus ’n subreus wat van die hoofreeks af wegbeweeg. Ná sy rooireusfase sal dit ’n witdwerg word. Sy ligsterkte is tans 10 000 keer dié van die Son en sy effektiewe temperatuur 22 570 K; dit gee daaraan die blouwit skynsel van ’n B-tipe ster.
Delta Crucis is ’n sterk kandidaat-Beta Cephei-veranderlike wat sy helderheid met ’n periode van 1,3 uur subtiel verander. Sy rotasiesnelheid is baie vinnig: sowat 210 km s-1.
↑ 1,0 1,1 Houk, Nancy; Cowley, A. P. (1978), Catalogue of two-dimensional spectral types for the HD stars: Declinations -90 to -53, 1, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1975mcts.book.....H
↑ Wielen, R. et al. (1999), Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions, Astronomisches Rechen-Institut Heidelberg, Bibcode: 1999VeARI..35....1W
↑ 4,0 4,1 4,2 de Geus, E. J.; de Zeeuw, P. T.; Lub, J. (June 1989), "Physical parameters of stars in the Scorpio-Centaurus OB association", Astronomy and Astrophysics 216 (1-2): 44–61, Bibcode: 1989A&A...216...44D
↑ 5,0 5,1 Gutierrez-Moreno, Adelina; Moreno, Hugo (June 1968), "A photometric investigation of the Scorpio-Centaurus association", Astrophysical Journal Supplement 15: 459, doi:10.1086/190168, Bibcode: 1968ApJS...15..459G
↑ 6,0 6,1 Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society 410 (1): 190–200, doi:10.1111/j.1365-2966.2010.17434.x, Bibcode: 2011MNRAS.410..190T
↑ Underhill, A. B. et al. (November 1979), "Effective temperatures, angular diameters, distances and linear radii for 160 O and B stars", Monthly Notices of the Royal Astronomical Society 189: 601–605, doi:10.1093/mnras/189.3.601, Bibcode: 1979MNRAS.189..601U
↑ Sokolov, N. A. (May 1995), "The determination of T_eff_ of B, A and F main sequence stars from the continuum between 3200 A and 3600 A", Astronomy and Astrophysics Supplement 110: 553, Bibcode: 1995A&AS..110..553S
↑ 9,0 9,1 (1970) “A catalogue of stellar rotational velocities”. Contributi Osservatorio Astronomico di Padova in Asiago 239 (1).
↑ 10,0 10,1 Telting, J. H. et al. (June 2006), "A high-resolution spectroscopy survey of β Cephei pulsations in bright stars", Astronomy and Astrophysics 452 (3): 945–953, doi:10.1051/0004-6361:20054730, Bibcode: 2006A&A...452..945T
↑ "HD 106490 – Variable Star of beta Cep type", SIMBAD Astronomical Database (Centre de Données astronomiques de Strasbourg), http://simbad.u-strasbg.fr/sim-id.pl?protocol=html&Ident=delta+crucis, besoek op 2005-11-05
Delta Crucis op WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Artikels en foto's
Koördinate: 12h 15m 08.71673s, −58° 44′ 56.1369″
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Die bladsy is laas op 12 Julie 2019 om 17:21 bygewerk.