New light on post-maximum oscillations of novae

Details New light on post-maximum oscillations of novae New light on post-maximum oscillations of novae

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...257..599b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 257, no. 2, p. 599-602.

Astronomy and Astrophysics

Astrophysics

14

Light Curve, Novae, Stellar Evolution, Stellar Oscillations, Stellar Structure, Dynamic Characteristics, Optical Thickness, Radial Velocity

Scientific paper

Post-optical maximum oscillations of classical novae and their empirical
characteristics are studied. Particular attention is given to GK Persei
radial velocity oscillations of the Orion absorption component which
appear to have minima for only each second light curve maximum. Possible
interpretations of the phenomenon are discussed.

Affiliated with

Also associated with

No associations

Rating

New light on post-maximum oscillations of novae 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 New light on post-maximum oscillations of novae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New light on post-maximum oscillations of novae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1731853