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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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Member of following groups:
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Observation and Astrometry data
| Constellation: | Baleine |
| Right ascension: | 01h07m44.60s |
| Declination: | -04°44'43.1" |
| Apparent magnitude: | 7.723 |
| Distance: | 571.429 parsecs |
| Proper motion RA: | 55.3 |
| Proper motion Dec: | -38.6 |
| B-T magnitude: | 9.376 |
| V-T magnitude: | 7.86 |
Catalogs and designations:
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INHABITED SKY
