Optical/IR observations of H1743-322

Details Optical/IR observations of H1743-322 Optical/IR observations of H1743-322

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..577....1b&link_type=abstract

The Astronomer's Telegram, #577

Astronomy and Astrophysics

Astronomy

Infra-Red, Optical, Binaries, Black Holes, Transients

Scientific paper

We obtained a 30m exposure in I and K of H1743-322, using the SMARTS consortium 1.3m and ANDICAM instrument at Cerro Tololo Interamerican Observatory, beginning at UT 00:36 August 12, 2005. We see no evidence for a rise in either band, to limits of I~22 and K~15. These limits are ~1.5 magnitudes fainter than was observed in April 2003 near the peak of the last outburst. Further observations to this depth are planned.

Affiliated with

Also associated with

No associations

Rating

Optical/IR observations of H1743-322 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 Optical/IR observations of H1743-322, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical/IR observations of H1743-322 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1347765