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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.
| Photoelectric Photometry of Stars in the Orion Standard Region
Magnitudes and color indices in the Vilnius seven-color photometricsystem are given for 108 stars in the Orion standard region around theOrion Belt and the star lambda Orionis. New spectral and luminosityclasses, estimated from the photometric data, are given for some of thestars.
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Datos observacionales y astrométricos
| Constelación: | Ballena |
| Ascensión Recta: | 00h54m43.43s |
| Declinación: | -07°14'17.8" |
| Magnitud Aparente: | 9 |
| Movimiento Propio en Ascensión Recta: | 57.4 |
| Movimiento Propio en Declinación: | 8.6 |
| B-T magnitude: | 9.563 |
| V-T magnitude: | 9.047 |
Catálogos y designaciones:
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