Study of Pre-Main Sequence Stars Born in LDN 1251

Details Study of Pre-Main Sequence Stars Born in LDN 1251 Study of Pre-Main Sequence Stars Born in LDN 1251

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cokon.103...27e&link_type=abstract

Communications of the Konkoly Observatory, Hungary Proceedings of the conference: 'The interaction of stars with their environme

Physics

4

Scientific paper

We observed the spectra of Hα emission stars in the molecular cloud L1251 using the CAFOS spectrograph on the 2.2 m telescope of Calar Alto Observatory. We found 7 pre-main sequence stars born in the cloud and determined their spectral and luminosity classes. These spectroscopic data, supplemented with near-infrared (JHK) magnitudes allowed us to place these stars in the HR diagram. This paper discusses the evolutionary status of star formation in LDN 1251.

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