IRAS observations of SS Cygni and other dwarf novae

Details IRAS observations of SS Cygni and other dwarf novae IRAS observations of SS Cygni and other dwarf novae

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987obs...107...72j&link_type=abstract

The Observatory, vol. 107, p. 72-74 (1987)

Physics

10

Scientific paper

SS Cygni was detected in IRAS bands I and II during an outburst. The
most likely origin of the infrared emission is circumstellar dust heated
by the enhanced UV flux during outburst.

Affiliated with

Also associated with

No associations

Rating

IRAS observations of SS Cygni and other dwarf 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 IRAS observations of SS Cygni and other dwarf novae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and IRAS observations of SS Cygni and other dwarf novae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1349423