Infrared flaring of the potential gamma-ray source QSO B0133+47

Details Infrared flaring of the potential gamma-ray source QSO B0133+47 Infrared flaring of the potential gamma-ray source QSO B0133+47

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1874....1c&link_type=abstract

The Astronomer's Telegram, #1874

Astronomy and Astrophysics

Astronomy

3

Infra-Red, Gamma Ray, Agn, Quasars

Scientific paper

We call attention on our recent observations of QSO B0133+47 with the
Cananea NIR camera (CANICA) on the 2.1m telescope at the Observatorio
Astrofísico Guillermo Haro. We found this quasar to show fluxes
2.5 magnitudes brighter than 2MASS values, of epoch 1999, but
undergoing a rapid decline.

Affiliated with

Also associated with

No associations

Rating

Infrared flaring of the potential gamma-ray source QSO B0133+47 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 Infrared flaring of the potential gamma-ray source QSO B0133+47, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Infrared flaring of the potential gamma-ray source QSO B0133+47 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-962399