Black Hole Candidate XTE J1859+226 in the Low/Hard State

Details Black Hole Candidate XTE J1859+226 in the Low/Hard State Black Hole Candidate XTE J1859+226 in the Low/Hard State

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000atel...60....1m&link_type=abstract

The Astronomer's Telegram, #60

Astronomy and Astrophysics

Astronomy

2

Radio, Optical, X-Ray, Request For Observations, Black Holes, Transients

Scientific paper

Recent flaring activity of this source in the optical (Casares et al. 2000, IAUC #7451) has motivated a public RXTE TOO observation on 8 July 2000. XTE J1859+226 is a known X-ray nova that reached 1.4 Crab in the RXTE/ASM in October 1999 (Smith 1999, ATEL #47). During that outburst the source exhibited 150 and 187 Hz quasi-periodic oscillations (Cui et al. 2000, ApJ 535, L123) and radio emission (Pooley & Hjellming, IAUC #7278).

Affiliated with

Also associated with

No associations

Rating

Black Hole Candidate XTE J1859+226 in the Low/Hard State 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 Black Hole Candidate XTE J1859+226 in the Low/Hard State, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Black Hole Candidate XTE J1859+226 in the Low/Hard State will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1718139