Detection of both soft and hard X-ray emission from SS Cygni with ANS

Details Detection of both soft and hard X-ray emission from SS Cygni with ANS Detection of both soft and hard X-ray emission from SS Cygni with ANS

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....63l...1h&link_type=abstract

Astronomy and Astrophysics, vol. 63, no. 1-2, Feb. 1978, p. L1-L3.

Astronomy and Astrophysics

Astronomy

27

Novae, Satellite Observation, Spaceborne Astronomy, X Ray Sources, Astronomical Netherlands Satellite, Satellite-Borne Instruments

Scientific paper

The dwarf nova SS Cygni was observed twice with the X-ray instruments aboard the Astronomical Netherlands Satellite ANS. A soft (0.16-0.284 keV) and a hard (1-7 keV) X-ray signal were detected while SS Cygni was in its quiescent optical state. The discovery of hard X-ray emission suggests that SS Cygni is a source similar to the AM Her/3U 1809+50 system.

Affiliated with

Also associated with

No associations

Rating

Detection of both soft and hard X-ray emission from SS Cygni with ANS 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 Detection of both soft and hard X-ray emission from SS Cygni with ANS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of both soft and hard X-ray emission from SS Cygni with ANS will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1033898