BD + 24 deg 676 - an intermediate-mass, pre-main-sequence star

Details BD + 24 deg 676 - an intermediate-mass, pre-main-sequence star BD + 24 deg 676 - an intermediate-mass, pre-main-sequence star

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..754w&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, July 1990, p. 754-757.

Astronomy and Astrophysics

Astronomy

6

Astronomical Spectroscopy, Mass Distribution, Pre-Main Sequence Stars, Star Formation, Stellar Spectrophotometry, T Tauri Stars, Balmer Series, Near Infrared Radiation, Ultraviolet Radiation

Scientific paper

An analysis of the optical spectrum and UBVRIJHKL photometry of BD + 24 deg 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 deg 676 is an intermediate-mass, premain-sequence star in the Taurus-Auriga region.

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