LkH-alpha 324, an interesting young star - The investigation continues

Details LkH-alpha 324, an interesting young star - The investigation continues LkH-alpha 324, an interesting young star - The investigation continues

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..544k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, June 1991, p. 544-547. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Early Stars, H Alpha Line, Light Curve, Stellar Magnitude, Variable Stars, Stellar Luminosity, Stellar Spectra, Stellar Spectrophotometry

Scientific paper

The stellar magnitudes of LkH-alpha 324 are presented on the basis of a series of photographic plates made during 1898-1984, as well as results of photoelectric UBV observations of the young star conducted during 1985-1990. It is inferred from a photometric behavior analysis that LkH-alpha 324 may belong to the group of young eruptive objects of the EX type (EXors). In December 1988 LkH-alpha 324 was classified as approximately F3; its hydrogen emission spectrum was found to decrease with time.

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