X-ray and UV observations of the low mass X-ray binary AC211 in the globular cluster M15

Details X-ray and UV observations of the low mass X-ray binary AC211 in the globular cluster M15 X-ray and UV observations of the low mass X-ray binary AC211 in the globular cluster M15

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261..351i&link_type=abstract

The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu

Physics

1

Scientific paper

We present X-ray and UV observations of the low-mass X-ray binary system X2127+119 (AC211), one of the few X-ray binary systems that is associated with a globular cluster. Our observations further strengthen the case that the X-ray emission from AC211 originates in an Accretion Disc Corona (ADC). The UV observations show that the UV continuum emission originates of the system, namely the accretion disc. In addition, we present the first ever detection of a C IV line at 1550 Å, which exhibits a prominent P Cygni profile.

Affiliated with

Also associated with

No associations

Rating

X-ray and UV observations of the low mass X-ray binary AC211 in the globular cluster M15 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 X-ray and UV observations of the low mass X-ray binary AC211 in the globular cluster M15, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray and UV observations of the low mass X-ray binary AC211 in the globular cluster M15 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1087658