Published March 20, 2010
| Published
Journal Article
Open
J16021+3326: New Multi-Frequency Observations Of a Complex Source
Chicago
An error occurred while generating the citation.
Abstract
We present multi-frequency Very Long Baseline Array observations of J16021+3326. These observations, along with variability data obtained from the Owens Valley Radio Observatory candidate gamma-ray blazar monitoring program, clearly indicate that this source is a blazar. The peculiar characteristic of this blazar, which daunted previous classification attempts, is that we appear to be observing down a precessing jet, the mean orientation of which is aligned with us almost exactly.
Additional Information
© 2010 American Astronomical Society. Received 2009 December 28; accepted for publication 2010 January 28; published 2010 February 25. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Facilities: VLBAAttached Files
Published - Tremblay2010p7391Astrophys_J.pdf
Files
Tremblay2010p7391Astrophys_J.pdf
Files
(1.1 MB)
| Name | Size | Download all |
|---|---|---|
|
md5:e810c3349755a173676b22b1cb622cd1
|
1.1 MB | Preview Download |
Additional details
- Eprint ID
- 17840
- Resolver ID
- CaltechAUTHORS:20100401-113556279
- Created
-
2010-04-01Created from EPrint's datestamp field
- Updated
-
2021-11-08Created from EPrint's last_modified field