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1--4 MU M Spectroscopy of Very Red Stars Found in an I-Band Objective Prism Survey
We present the 1.2--4.2 mu m spectroscopy of stars found in an objectiveprism survey of the galactic plane by Stephenson (1992, AAA 55.002.010).These stars were thought by Stephenson to be heavily reddened byinterstellar absorption. However, almost all of them have turned out tobe late-type stars with clear 2.3 mu m CO absorption, which means thatthey are intrinsically red as well. A few stars have AV ~ 9, but mostof them are only moderately reddened (AV = 1--5).
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Membro dei seguenti gruppi:
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Osservazione e dati astrometrici
| Costellazione: | Auriga |
| Ascensione retta: | 06h34m42.18s |
| Declinazione: | +29°22'13.8" |
| Magnitudine apparente: | 8.423 |
| Moto proprio RA: | -13.3 |
| Moto proprio Dec: | -2.4 |
| B-T magnitude: | 10.536 |
| V-T magnitude: | 8.598 |
Cataloghi e designazioni:
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