J/A+A/465/993       Spectral atlas of massive stars around He I   (Groh+, 2007)

Spectral atlas of massive stars around He I 10830Å. Groh J.H., Damineli A., Jablonski F. <Astron. Astrophys. 465, 993 (2007)> =2007A&A...465..993G 2007A&A...465..993G
ADC_Keywords: Stars, early-type ; Stars, Be ; Spectra, infrared Keywords: atlases - stars: emission-line, Be - stars: Wolf-Rayet - stars: winds, outflows - stars: early-type Abstract: We present a digital atlas of peculiar, high-luminosity massive stars in the near-infrared region (10470-11000Å) at medium resolution (R∼7000). The spectra are centered around HeI 10830Å, which is formed in the wind of those stars, and is a crucial line to obtain their physical parameters. The instrumental configuration also sampled a rich variety of emission lines of FeII, MgII, CI, NI, and Paγ. Secure identifications for most spectral lines are given, based on synthetic atmosphere models calculated by our group. We also propose that two unidentified absorption features have interstellar and/or circumstellar origin. For the strongest one (10780Å) an empirical calibration between E(B-V) and equivalent width is provided. The atlas displays the spectra of massive stars organized in four categories, namely Be stars, OBA Iape (or luminous blue variables, LBV candidates and ex/dormant LBVs), OB supergiants and Wolf-Rayet stars. For comparison, the photospheric spectra of non emission-line stars are presented. Selected LBVs were observed in different epochs from 2001 to 2004, and their spectral variability reveals that some stars, such as eta Car, AG Car and HR Car, suffered dramatic spectroscopic changes during this time interval. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 181 40 Basic data for the program stars refs.dat 72 15 References sp/* . 60 Individual spectra -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Type Type (class) of star (1) 3- 13 A11 --- Star Star name 15- 20 I6 --- HD ? HD number 22- 23 I2 h RAh Right ascension (J2000) 25- 26 I2 min RAm Right ascension (J2000) 28- 31 F4.1 s RAs Right ascension (J2000) 33 A1 --- DE- Declination sign (J2000) 34- 35 I2 deg DEd Declination (J2000) 37- 38 I2 arcmin DEm Declination (J2000) 40- 43 F4.1 arcsec DEs Declination (J2000) 45- 60 A16 --- SpType Spectral type 61- 63 I3 km/s vsini ? Projected rotational velocity, for Be stars only 65 A1 --- Neb? [y/n] Presence of a circumstellar nebula, for LBVs and related objects only 67- 82 A16 --- Refs References 84- 96 A13 --- FileName1 First spectrum filename in subdirectory sp 98-107 A10 "YYYY/MM/DD" ObsDate1 First observation date 109-120 A12 --- FileName2 Second spectrum filename in subdirectory sp 122-131 A10 "YYYY/MM/DD" ObsDate2 Second observation date 133-145 A13 --- FileName3 Third spectrum filename in subdirectory sp 147-156 A10 "YYYY/MM/DD" ObsDate3 Third observation date 158-170 A13 --- FileName4 Fourth spectrum filename in subdirectory sp 172-181 A10 "YYYY/MM/DD" ObsDate4 Fourth observation date -------------------------------------------------------------------------------- Note (1): Type as follows: 1 = Be stars 2 = LBVs, LBV candidates and ex/dormant LBVs 3 = OB Supergiants 4 = Wolf-Rayet stars -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- Ref Reference code 8- 26 A19 --- BibCode BibCode 28- 48 A21 --- Aut Author's name 51- 72 A22 --- Com Comments -------------------------------------------------------------------------------- Acknowledgements: Jose Henrique Groh, jgroh(at)mpifr-bonn.mpg.de
(End) Patricia Vannier [CDS] 05-Apr-2007
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line