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BD + 24 degree 676 - An intermediate-mass, pre-main-sequence star

Journal Article · · Publications of the Astronomical Society of the Pacific; (USA)
OSTI ID:6368570
; ;  [1]
  1. Colorado Univ., Boulder (USA) Ne York State Univ., Stony Brook (USA)
An analysis of the optical spectrum and UBVRIJHKL photometry of BD + 24{degree} 676 indicates that it is a heavily reddened emission-line star of spectral type A3. The star has substantial near-IR and UV excesses. A comparison with previous photometry suggests that this star may be variable. It is suggested that BD + 24{degree} 676 is an intermediate-mass, premain-sequence star in the Taurus-Auriga region. 12 refs.
OSTI ID:
6368570
Journal Information:
Publications of the Astronomical Society of the Pacific; (USA), Journal Name: Publications of the Astronomical Society of the Pacific; (USA) Vol. 102; ISSN PASPA; ISSN 0004-6280
Country of Publication:
United States
Language:
English