IGR J06074+2205 is a Be X-ray Binary

Details IGR J06074+2205 is a Be X-ray Binary IGR J06074+2205 is a Be X-ray Binary

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..959....1t&link_type=abstract

The Astronomer's Telegram, #959

Astronomy and Astrophysics

Astronomy

2

X-Ray, Binaries, Black Holes, Neutron Stars, Transients, Variables

Scientific paper

The X-ray source IGR J06074+2205 was discovered using data from observations made by INTEGRAL in 2003 February. (Chenevez et al. 2004, ATEL#223). Two different sources in the 2 arcminute INTEGRAL error circle have been suggested as possible counterparts. The first is the radio source NVSS J060718 +220452 (Pooley et al. 2004, ATEL#226; Pandey et al. 2006), while the second possible counterpart is a Be star (Halpern & Tyagi 2005, ATEL#682; Masetti et al.

Affiliated with

Also associated with

No associations

Rating

IGR J06074+2205 is a Be X-ray Binary 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 IGR J06074+2205 is a Be X-ray Binary, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and IGR J06074+2205 is a Be X-ray Binary will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1242026