Evidence for an accretion disk in SMC X-1

Details Evidence for an accretion disk in SMC X-1 Evidence for an accretion disk in SMC X-1

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....61l..19v&link_type=abstract

Astronomy and Astrophysics, vol. 61, no. 3, Nov. 1977, p. L19-L22. Research supported by the Nederlandse Organisatie voor Zuive

Astronomy and Astrophysics

Astrophysics

33

Binary Stars, Neutron Stars, Stellar Spectrophotometry, X Ray Sources, Light Curve, Roche Limit, Stellar Evolution

Scientific paper

An analysis of five-color photometric observations of Sk 160 (SMC X-1)
gives evidence for the existence of an accretion disk around the neutron
star in this system. This supports the suggestion by Hutchings et al.
(1977) that the mass transfer in SMC X-1 occurs through Rochelobe
overflow.

Affiliated with

Also associated with

No associations

Rating

Evidence for an accretion disk in SMC X-1 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 Evidence for an accretion disk in SMC X-1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evidence for an accretion disk in SMC X-1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1130627