Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1103....1k&link_type=abstract
The Astronomer's Telegram, #1103
Astronomy and Astrophysics
Astronomy
1
X-Ray, Transients
Scientific paper
On June 10th, 2007 at 20:52:26 UT, the Swift BAT instrument triggered on the X-ray transient source SWIFT J195509.6+261406, which was initially thought to a GRB (Pagani et al., GCN #6489), but is more likely to be be a galactic X-ray transient (Markwardt et al., ATEL #1102). In the field of this transient, we detect a previously unknown variable X-ray source at the following location: RA (J2000) = 19h 54m 56.78s, Dec (J2000) = +26d 13' 01.13", with error radius of 3.7 arcsec (90% uncertainty), designated SWIFT J195456.7+261301.
Evans Paul
Kennea Jaime A.
Markwardt Craig B.
Pagani Chiara
Tagliaferri Giampiero
No associations
LandOfFree
SWIFT J195456.7+261301: a flaring coronal X-ray emitting star 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 SWIFT J195456.7+261301: a flaring coronal X-ray emitting star, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SWIFT J195456.7+261301: a flaring coronal X-ray emitting star will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-875965