Reasons why nova FH Serpentis 1970 probably had a total luminosity above the Eddington limit during its outburst

Details Reasons why nova FH Serpentis 1970 probably had a total luminosity above the Eddington limit during its outburst Reasons why nova FH Serpentis 1970 probably had a total luminosity above the Eddington limit during its outburst

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...179..164f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 179, no. 1-2, June 1987, p. 164-166.

Astronomy and Astrophysics

Astrophysics

11

Novae, Stellar Luminosity, Stellar Mass Ejection, Stellar Winds, Kinetic Energy, Optical Thickness, Photosphere

Scientific paper

There is good evidence that novae in general and nova FH Ser 1970 in
particular have (had) optically thick winds for a long time after the
initial explosion. If this interpretation is accepted the total kinetic
and radiative flux of FH Ser appears to have stayed well above the
Eddington limit for about two months after optical maximum.

Affiliated with

Also associated with

No associations

Rating

Reasons why nova FH Serpentis 1970 probably had a total luminosity above the Eddington limit during its 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 Reasons why nova FH Serpentis 1970 probably had a total luminosity above the Eddington limit during its outburst, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Reasons why nova FH Serpentis 1970 probably had a total luminosity above the Eddington limit during its outburst will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1813261