Distance to the Serpens cloud. II

Details Distance to the Serpens cloud. II Distance to the Serpens cloud. II

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...243..139d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 243, no. 1, March 1991, p. 139-142. COSNET-supported research.

Astronomy and Astrophysics

Astrophysics

70

Dark Matter, Infrared Photometry, Molecular Clouds, Reflection Nebulae, Stellar Luminosity, Data Bases, H Alpha Line, Near Infrared Radiation, Star Formation, Stellar Mass

Scientific paper

Near IR photometry of stars with reflection nebulosity (R-stars) associated with the Serpens dark cloud is presented. A reexamination of earlier slit spectrograms of four bright R-stars confirms the luminosity classes and spectral types previously reported. In an attempt to detect the star responsible for the red nebulosity in the vicinity of star 17, ten IR sources are reported and their probable natures are discussed. It is shown that this study has significantly extended the list of well-observed R-stars and consequently it is believed that the distance estimate given for the Serpens dark cloud is the best currently available.

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