Radio Emission from the X-ray transient XTE J1550-564

Details Radio Emission from the X-ray transient XTE J1550-564 Radio Emission from the X-ray transient XTE J1550-564

2001-02-05

arxiv.org/abs/astro-ph/0102070v1

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures. Proceedings of the 4th INTEGRAL Workshop (Alicante 2000), to be published in ESA-SP (2001)

Scientific paper

We report multifrequency radio observations of XTE J1550-564 obtained with the Molonglo Observatory Synthesis Telescope and the Australia Telescope Compact Array at the time of its discovery and subsequent hard and soft X-ray outburst in 1998 September. A large radio flare was observed, peaking about 1.8 days after the X-ray flare. In addition, we present Australian Long Baseline Array images obtained shortly after the maximum of the radio flare which show evolving structure. The apparent separation velocity of the two outermost components is v>2c.

Affiliated with

Also associated with

No associations

Rating

Radio Emission from the X-ray transient XTE J1550-564 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 Radio Emission from the X-ray transient XTE J1550-564, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio Emission from the X-ray transient XTE J1550-564 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-104436