DOI: 10.5281/zenodo.14050100
title: HI line observations of 290 evolved stars made with the Nancay Radio Telescope - I. Data: online Tables

description: --- Table B.1: Clear NRT HI detections - basic data 

Description of the columns:

(1)  Name: common catalogue name of the target.   An ^n after a name indicates that it is clearly not an AGB star,   a ^d that we consider its classification as an AGB to be dubious,    and a ^* indicates that notes on the object can be found in Appendix A;(2,3) RA,DEC: literature right ascension and declination of the target from Gaia EDR 3,   for epoch J2000.0;(4) Type: target type.   Primarily the variability type as listed in Version 5.1 of the General Catalogue of Variable Stars,   GCVS (A description of GCVS types is given in https://cdsarc.u-strasbg.fr/ftp/cats/B/gcvs/vartype.txt),  but if an object is not included in the GCVS, other identifiers are listed in brackets:   HPM = high proper motion star, (OH/IR) = OH/IR maser,  LPVc = long-period variable candidate,   PN = planetary nebula, pPN = proto-planetary nebula, and post-AGB star;(5,6) Spec & ref: spectral type of the star, followed by its literature reference,   as retrieved from the SIMBAD database. If none was listed there, the reference is noted as 'SIMBAD';(7,8) Teff & ref: effective temperature of the star, in K, followed by its literature reference; (9) d: distance of the target, based on its parallax (mainly from the Gaia EDR3), in pc.  If no Gaia parallax was available a reference to the distance we adopted is given in Appendix A  (for RAFGL 3099, mu Cep, and V Peg);(10) Vlit: published radial velocity of the target in the LSR reference frame, in km/s;(11) Vexp: literature expansion velocity measured from CO or OH 1612 MHz line observations, in km/s.   If a pair of values was published for a two-velocity component CO line fit, the largest value is listed here;(12) ref: literature references to the published Vlit and Vexp values; (13) line: spectral line on which the published radial velocity measurement (Vlit) was based;(14,15) Mdot & ref: literature mass loss rates, in solar masses per year,   followed by its literature reference.

Notes to Table B.1:

References: see Table B.1 in the Astronomy & Astrophysics paper.

--- Table B.2: Clear NRT HI detections - HI data 

Description of the columns:

(1) Name: common catalogue name of the target.   A ^T after a name indicates that HI line parameters are based on a  'total' spectrum, whereas   a ^P indicates that a 'peak' spectrum was used.   An ^n indicates that it is clearly not an AGB star,   a ^d that we consider its classification as an AGB to be dubious,    and a ^* indicates that notes on the object can be found in Appendix A;(2) VHI: our central radial velocity in the LSR reference frame of the Gaussian fitted   to the HI profile, in km/s.(3) FWHM: our full width half maximum of the Gaussian fitted to the HI line profile, in km/s;(4) Speak: our peak flux density of the HI line profile, in Jy;(5) diam: our estimated angular size of the HI CSE in the east-west direction, in arcmin;(6) FHI: our integrated line flux of the HI profile, in Jy km/s;(7) MHI: our total HI mass, in Msun;(8) HI ref: references to previously published HI studies,  see Table B.2 in the Astronomy & Astrophysics paper.

--- Table B.3: Possible NRT HI detections - basic data

Description of the columns:

(1)  Name: common catalogue name of the target.   An ^n after a name indicates that it is clearly not an AGB star,   a ^d that we consider its classification as an AGB to be dubious,    and a ^* indicates that notes on the object can be found in Appendix A;(2,3) RA,DEC: literature right ascension and declination of the target from Gaia EDR 3,   for epoch J2000.0;(4) Type: target type.   Primarily the variability type as listed in Version 5.1 of the General Catalogue of Variable Stars,   GCVS (A description of GCVS types is given in https://cdsarc.u-strasbg.fr/ftp/cats/B/gcvs/vartype.txt),  but if an object is not included in the GCVS, other identifiers are listed in brackets:   HPM = high proper motion star, (OH/IR) = OH/IR maser,  LPVc = long-period variable candidate,   PN = planetary nebula, pPN = proto-planetary nebula, and post-AGB star;(5,6) Spec & ref: spectral type of the star, followed by its literature reference,   as retrieved from the SIMBAD database. If none was listed there, the reference is noted as 'SIMBAD';(7,8) Teff & ref: effective temperature of the star, in K, followed by its literature reference; (9) d: distance of the target, based on its parallax (mainly from the Gaia ED33), in pc.  If no Gaia parallax was available a reference to the distance we adopted is given in Appendix A (for RAFGL 3099, mu Cep, and V Peg);(10) Vlit: published radial velocity of the target in the LSR reference frame, in km/s;(11) Vexp: literature expansion velocity measured from CO or OH 1612 MHz line observations, in km/s.   If a pair of values was published for a two-velocity component CO line fit, the largest value is listed here;(12) Mdot : literature mass loss rates, in solar masses per year, (13) line: spectral line on which the published radial velocity measurement (Vlit) was based;(14) ref: literature references to the published Vlit, Vexp and Mdot values; 

Notes to Table B.3:

References: see Table B.1 in the Astronomy & Astrophysics paper.

--- Table B.4: Possible NRT HI detections - HI data

Description of the columns:

See the description of the columns of Table B.2.

--- Online only Table 5: Upper limits to NRT HI lines 

Description of the columns:

(1)  Name: common catalogue name of the target.   An ^n after a name indicates that it is clearly not an AGB star,   a ^d that we consider its classification as an AGB to be dubious,    and a ^* indicates that notes on the object can be found in Appendix A;(2,3) RA,DEC: literature right ascension and declination of the target from Gaia EDR 3,   for epoch J2000.0;(4) Type: target type.   Primarily the variability type as listed in Version 5.1 of the General Catalogue of Variable Stars,   GCVS (A description of GCVS types is given in https://cdsarc.u-strasbg.fr/ftp/cats/B/gcvs/vartype.txt),  but if an object is not included in the GCVS, other identifiers are listed in brackets:   HPM = high proper motion star, (OH/IR) = OH/IR maser,  LPVc = long-period variable candidate,   PN = planetary nebula, pPN = proto-planetary nebula, and post-AGB star;(5,6) spec & ref: spectral type of the star, followed by its literature reference,   as retrieved from the SIMBAD database. If none was listed there, the reference is noted as 'SIMBAD';(7,8) Teff & ref: effective temperature of the star, in K, followed by its literature reference; (9) d: distance of the target, based on its parallax (mainly from the Gaia EDR3, in pc.  If no Gaia parallax was available a reference to the distance we adopted is given in Appendix A (for RAFGL 3099, mu Cep, and V Peg);(10) Vlit: published radial velocity of the target in the LSR reference frame, in km/s;(11) Vexp: literature expansion velocity measured from CO or OH 1612 MHz line observations, in km/s.   If a pair of values was published for a two-velocity component CO line fit, the largest value is listed here;(12) Mdot : literature mass loss rates, in solar masses per year, (13) ref: literature references for Vlit, Vexp and Mdot, as applicable;(14) line: spectral line on which the published radial velocity measurement (Vlit) was based;(15) Speak: peak flux density of our HI line profile, in Jy;(16) notes: 'old data' indicates objects observed only in 1992/1993, before the  renovation of the NRT;   'blue/red side' indicates that either the blue or red side of the HI profile could be used to measure   an upper limit to the line flux;(17) HI ref: references to previously published HI studies;

Notes to online only Table 5: 

HI references: see Table B.2 in the Astronomy & Astrophysics paper.Other references: see Table B.1 in the Astronomy & Astrophysics paper.

--- Online only Table 6: Confused NRT HI spectra

Description of the columns:

(1) Name: common catalogue name of the target. (2,3) RA, DEC: literature right ascension and declination of the target from Gaia EDR3,   for epoch J2000.0; (4) type: target type. Primarily the variability type as listed in Version 5.1 of the   General Catalogue of Variable Stars, GCVS; but if an object is not included in the GCVS,   other identifiers are listed in brackets:  HPM = high proper motion star, (OH/IR) = OH/IR maser,   LPVc = long-period variable candidate, PN = planetary nebula, pPN = proto-planetary nebula,   and post-AGB star; (5,6) spec & ref spectral type of the star, followed by its literature reference,  as retrieved from the SIMBAD database. If none was listed there, the reference is noted as 'SIMBAD'; (7,8) Vlit & ref: published radial velocity of the target in the LSR reference frame, in km/s; (9) line: spectral line on which the published radial velocity measurement (Vlit) was based; (10) notes: 'old data' denotes objects observed only in 1992/1993, before the renovation of the NRT (see Section 3), for which no observations in digital form are available; (11) HI ref: references to previously published HI studies.

Notes to online only Table 6:

HI references: see Table B.2 in the Astronomy & Astrophysics paper.Other references: see Table B.1 in the Astronomy & Astrophysics paper.