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Medium-Resolution Stellar Spectra in the L Band from 2400 to 3000 cm-1 (3.3 to 4.2 Microns) We present a brief atlas of L-band (3.3-4.2 μm) spectra for 42 starsplus the Sun and a sunspot observed at a resolving power of R~3000. Thiscontribution is intended to supplement our previous K-band, H-band, andJ-band spectral atlases. The L-band data, which cover some or all of the2400 to 3000 cm-1 (3.3-4.2 μm) region, are mainly forluminous late-type stars. In reducing these data, special care has beentaken to remove telluric features, especially water vapor. We identifytemperature- and luminosity-sensitive atomic and molecular indices toaid in the classification of stellar spectra in the L band. The data areavailable electronically.
| Colors, luminosities, and motions of the nearer G-type stars Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1964AJ.....69..570E&db_key=AST
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Gözlemler ve gökölçümü verileri
Takýmyýldýz: | Balina |
Sað Açýklýk: | 01h07m44.60s |
Yükselim: | -04°44'43.1" |
Görünürdeki Parlaklýk: | 7.723 |
Uzaklýk: | 571.429 parsek |
özdevim Sað Açýklýk: | 55.3 |
özdevim Yükselim: | -38.6 |
B-T magnitude: | 9.376 |
V-T magnitude: | 7.86 |
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