A Medium‐Resolution Near‐Infrared Spectral Library of Late‐Type Stars. I.
Author(s) -
V. D. Ivanov,
Marcia Rieke,
C. W. Engelbracht,
A. AlonsoHerrero,
G. H. Rieke,
K. L. Luhman
Publication year - 2004
Publication title -
the astrophysical journal supplement series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.546
H-Index - 277
eISSN - 1538-4365
pISSN - 0067-0049
DOI - 10.1086/381752
Subject(s) - bulge , stars , physics , astrophysics , globular cluster , spectral line , infrared , stellar classification , luminosity , spectral resolution , astronomy , population , galaxy , demography , sociology
We present an empirical infrared spectral library of medium resolution(R~2000-3000) H (1.6 micron) and K (2.2 micron) band spectra of 218 red stars,spanning a range of [Fe/H] from ~-2.2 to ~+0.3. The sample includes Galacticdisk stars, bulge stars from Baade's window, and red giants from Galacticglobular clusters. We report the values of 19 indices covering 12 spectralfeatures measured from the spectra in the library. Finally, we derivecalibrations to estimate the effective temperature, and diagnosticrelationships to determine the luminosity classes of individual stars fromnear-infrared spectra. This paper is part of a larger effort aimed at building a near-IR spectrallibrary to be incorporated in population synthesis models, as well as, attesting synthetic stellar spectra.Comment: 34 pages, 12 figures; accepted for publication at ApJS; the spectra are available from the authors upon reques
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom