J/A+AS/123/135     Spectral classifications of 180 IR stars     (Ginestet+ 1997)

Spectral classifications in the near infrared of stars with composite spectra. II. Study of a sample of 180 stars. Ginestet N., Carquillat J.M., Jaschek C., Jaschek M. <Astron. Astrophys. Suppl. Ser. 123, 135 (1997)> =1997A&AS..123..135G 1997A&AS..123..135G (SIMBAD/NED BibCode)
ADC_Keywords: Spectra, infrared ; MK spectral classification Keywords: stars: classification - infrared: stars - binaries: spectroscopic Abstract: A sample of 180 supposedly composite-spectrum stars has been studied on the basis of spectra obtained in the near infrared (8370-8780Å) at a dispersion of 33Å/mm. The objective was to study the cooler components of the systems. Of our sample, 120 are true composite spectra, 35 are hot spectra of types B, F and 25 are Am stars. We find a strong concentration of the cooler components of the composite spectra around G8III. In view of the difficulty of classifying composite spectra, because of the superposition of an early type dwarf and a late type giant or supergiant spectrum, we have made several tests to control the classification based upon the infrared region. Since all tests gave positive results, we conclude that our classifications can be considered as being both reliable and homogeneous. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 242 120 Classifications of the cool components, SP(IR), of stars with composite spectra table2.dat 55 60 Stars of the sample which exhibit a hot spectrum refs.dat 68 64 References -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- HD/BD HD of BD number of the star 10- 11 I2 h RAh Right ascension (J2000) 13- 14 I2 min RAm Right ascension (J2000) 16- 19 F4.1 s RAs Right ascension (J2000) 21 A1 --- DE- Declination sign 22- 23 I2 deg DEd Declination (J2000) 25- 26 I2 arcmin DEm Declination (J2000) 28- 29 I2 arcsec DEs Declination (J2000) 31- 35 F5.2 mag Vmag V magnitude 36 A1 --- u_Vmag Uncertainty flag on Vmag 38- 41 F4.2 mag B-V ? B-V color index 44- 54 A11 --- SpIR This work spectral type (1) 55 A1 --- n_SpIR [*] Note on the object (2) 57- 72 A16 --- Sp1 Spectral type 74- 91 A18 --- r_Sp1 References for spectral type (see refs.dat file) 93-106 A14 --- Sp2 Spectral type 107 A1 --- n_Sp2 [*] Note on the object (2) 108-125 A18 --- r_Sp2 References for spectral type (see refs.dat file) 127-142 A16 --- Sp3 Spectral type 144-160 A17 --- r_Sp3 References for spectral type (see refs.dat file) 162-173 A12 --- Sp4 Spectral type 175-190 A16 --- r_Sp4 References for spectral type (see refs.dat file) 192-197 A6 --- Sp5 Spectral type 199-213 A15 --- r_Sp5 References for spectral type (see refs.dat file) 215-225 A11 --- Sp6 Spectral type 227-242 A16 --- r_Sp6 References for spectral type (see refs.dat file) -------------------------------------------------------------------------------- Note (1): A - or + sign following the Sp(IR) luminosity class indicates that the object is probably slightly more or less luminous. Note (2): Individual notes: HD 18715: classification based on the cool component, since both components are well separated (8") HD 26630: standard MK G0 Ib HD 51250: standard of radial velocity HD 74395: standard MK G1 Ib HD 84367: the secondary is probably an Am star HD 197177: standard MK G8 IIb HD 199378: the authors suspect the object to be composite (G5III+A) HD 209278: visual binary, separated 3.7", but the classification is based on the combined light HD 212391: the classification is based on the spectrum of the cool star since the separation of 4.3" permits to observe individually each component. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- HD/BD HD or BD name 8- 12 F5.2 mag Vmag V magnitude 13 A1 --- u_Vmag Uncertainty flag on Vmag 14- 18 F5.2 mag B-V ? B-V color index 21- 36 A16 --- Sp Spectral type 37 A1 --- n_Sp [*] * when individual note (1) 39- 53 A15 --- SpIR This work spectral type 55 A1 --- n_SpIR [*] * when individual note (1) -------------------------------------------------------------------------------- Note (1): HD 14262: also classed A7V (Palmer et al., 1968RGOB..135..385P 1968RGOB..135..385P) HD 16646: F4Vwl (Abt, 1984ApJ...285..247A 1984ApJ...285..247A) HD 24346: slightly weak-lined F type star (Bidelman, 1988PASP..100.1084B 1988PASP..100.1084B) HD 41724: Am (Bidelman, 1988PASP..100.1084B 1988PASP..100.1084B; Carquillat et al., 1988A&AS...75..305C 1988A&AS...75..305C) HD 48953: G5Ia+A5V (Markowitz, 1969, Ph.D thesis, Ohio State Univ.), Ap Sr-Eu (Bidelman, 1988PASP..100.1084B 1988PASP..100.1084B) HD 51565: G2IIIe (Kuhi, 1963PASP...75..448K 1963PASP...75..448K); Am (Smith, 1973ApJS...25..277S 1973ApJS...25..277S) HD 60178: Castor B HD 68119: larger proper motion (CDS); moderatly weak-lines F type star (Bidelman, 1988PASP..100.1084B 1988PASP..100.1084B) HD 76369: appears normal (Bidelman, 1988PASP..100.1084B 1988PASP..100.1084B) HD 76370: G5III+A0V (Markovitz, 1969, Ph.D thesis, Ohio State Univ.) HD 83270: Am (Bidelman, 1988PASP..100.1084B 1988PASP..100.1084B; Ginestet et al., 1991A&AS...91..265G 1991A&AS...91..265G) HD 83808: SB2. The dominating spectrum is that of an Am star, the secondary could be a late F type. Also classified A1V+F6II (Markovitz, 1969, Ph.D thesis, Ohio State Univ.) and A5V+F8III (Parsons, 1983ApJS...53..553P 1983ApJS...53..553P) HD 86167: Am (Abt, 1984ApJ...285..247A 1984ApJ...285..247A) HD 88923: F2Vwl (Abt, 1984ApJ...285..247A 1984ApJ...285..247A) HD 91172: Fm Delta Del (Houk & Smoth-Moore, 1988 Catalogue III/133) HD 97336: Bidelman (1988PASP..100.1084B 1988PASP..100.1084B): "not composite" HD 107054: A8V (Palmer et al., 1968RGOB..135..385P 1968RGOB..135..385P); A9IVn (Gray & Garrison, 1989ApJS...69..301G 1989ApJS...69..301G) HD 114519: RS CVn (SB2), Algol eclipsing type binary; Batten et al (19899PDAO...17....1B): F4IV-V+K0IV; Strassmeier & Fekel (1990A&A...230..389S 1990A&A...230..389S): F6IV+G8IV. The spectrum is difficult to classify because of the high rotation, but the Ti/Fe ratios suggest a secondary at least as late as K4. HD 120544: F7V (Cowley, 1976PASP...88...95C 1976PASP...88...95C) HD 123102: A9IV (Abt, 1981ApJS...45..437A 1981ApJS...45..437A); visual double, sep. 13.5" HD 187949: A1V+F4III: (Markowitz, 1969Ph.D thesis, Ohio State Univ.); Algol type eclipsing binary. HD 206088: F0p Sr (Bertaud, 1959JO.....42...45B 1959JO.....42...45B) HD 208132: Am (Bertaud, 1965JO.....48..211B 1965JO.....48..211B) HD 209790: Am (Slettebak, 1963ApJ...138..118S 1963ApJ...138..118S) HD 209791: F7V (Slettebak, 1963ApJ...138..118S 1963ApJ...138..118S) HD 214605: Am (Bidelman, 1988PASP..100.1084B 1988PASP..100.1084B) HD 239746: B2V comp.? (Niedzielski & Muciek, 1988AcA....38..225N 1988AcA....38..225N) HD 239933: is not in the CDS database -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 A18 --- Ref Code of the reference 20- 38 A19 --- BibCode Bibcode of the reference 40- 68 A29 --- Comm Comment -------------------------------------------------------------------------------- References: Ginestet et al. Paper I. 1994A&AS..108..359G 1994A&AS..108..359G
(End) Patricia Bauer [CDS] 27-Sep-1996
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