Near-infrared classification spectroscopy: H-band spectra of fundamental MK standards

Citation
Mr. Meyer et al., Near-infrared classification spectroscopy: H-band spectra of fundamental MK standards, ASTROPHYS J, 508(1), 1998, pp. 397-409
Citations number
47
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
508
Issue
1
Year of publication
1998
Part
1
Pages
397 - 409
Database
ISI
SICI code
0004-637X(19981120)508:1<397:NCSHSO>2.0.ZU;2-3
Abstract
We present a catalog of H-band spectra for 85 stars of approximately solar abundance observed at a resolving power of 3000 with the KPNO Mayall 4 m Fo urier Transform Spectrometer. The atlas covers spectral types O7-M5 and lum inosity classes I-V as defined in the MK system. We identify both atomic an d molecular indices and line ratios that are temperature and luminosity sen sitive, allowing spectral classification to be carried out in the H-band. T he line ratios permit spectral classification in the presence of continuum excess emission, which is commonly found in pre-main-sequence or evolved st ars. We demonstrate that with spectra of R = 1000 obtained at signal-to-noi se ratio >50, it is possible to derive spectral types within +/-2 subclasse s for late-type stars. These data are available electronically through the Astronomical Data Center in addition to being served on the World Wide Web.