The outburst of V 1057 CYG

Details The outburst of V 1057 CYG The outburst of V 1057 CYG

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976s%26w....15..281b&link_type=abstract

Sterne und Weltraum, vol. 15, Sept. 1976, p. 281-285. In German.

Astronomy and Astrophysics

Astronomy

Infrared Astronomy, Stellar Evolution, Stellar Luminosity, T Tauri Stars, Variable Stars, A Stars, Atmospheric Models, Flares, Main Sequence Stars, Photosphere, Stellar Mass, Stellar Models, Stellar Temperature

Scientific paper

The behavior of the variable star V 1057 Cyg, which increased its brightness during an interval of a few months by almost six stellar magnitudes, is similar to that of the star FU Ori in 1936/37. It is known that V 1057 Cyg was a T Tauri star before the outburst. An analysis of the characteristics of the outburst of V 1057 Cyg provides, therefore, important information for a study of T Tauri stars and the theory of stellar development. Attention is given to details concerning the discovery of V 1057 Cyg, its study, the behavior of V 1057 Cyg before the outburst, models of the photosphere, infrared observations, the stellar mass, and an interpretation of the observed phenomena

Affiliated with

Also associated with

No associations

Rating

The outburst of V 1057 CYG does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The outburst of V 1057 CYG, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The outburst of V 1057 CYG will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1416606