The recurrent nova V394 Coronae Austrinae - The 1987 outburst

Details The recurrent nova V394 Coronae Austrinae - The 1987 outburst The recurrent nova V394 Coronae Austrinae - The 1987 outburst

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.236..611s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 236, Feb. 1, 1989, p. 611-619.

Astronomy and Astrophysics

Astronomy

21

Emission Spectra, Novae, Stellar Spectra, Astronomical Photometry, Astronomical Spectroscopy, H Alpha Line, Light Curve

Scientific paper

Optical and infrared observations of the 1987 outburst of the recurrent nova V394 Coronae Austrinae are reported. The amplitude of the outburst (Delta V of about 11 mag) is comparable to that of classical novae. The fast optical decline rate and the gross spectral characteristics of V394 CrA closely resemble those of U Sco. Compared to U Sco, the broad emission bands in the early decline are slightly narrower, and the late optical decline and spectral development are slower. Implications for thermonuclear runaway models are mentioned.

Affiliated with

Also associated with

No associations

Rating

The recurrent nova V394 Coronae Austrinae - The 1987 outburst 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 recurrent nova V394 Coronae Austrinae - The 1987 outburst, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The recurrent nova V394 Coronae Austrinae - The 1987 outburst will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1885293