VLA observation of NVSS J191656+051126

Details VLA observation of NVSS J191656+051126 VLA observation of NVSS J191656+051126

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...350..753l&link_type=abstract

Astronomy and Astrophysics, v.350, p.753-756 (1999)

Astronomy and Astrophysics

Astrophysics

Radio Continuum: General

Scientific paper

We present new Very Large Array (VLA) radio observations in X, U, K, and Q bands (from 8.4 to 43 GHz) of a serendipitously detected radio source observed during a campaign on dMe stars in April 1996. Cross correlating the coordinates, we found an entry in the NRAO NVSS survey catalog at 1.4 GHz. According to the rules of this survey, we named this serendipitous source ``NVSS J191656+051126''. No optical or X-ray counterpart could be identified, while we find that the IRAS point source IRAS 19145+0505 could be the IR counterpart. Using the radio data, we determined that the source spectral index is compatible with synchrotron emission mechanism. We have also investigated the structure of the source that is resolved into two components and their time variability.

Affiliated with

Also associated with

No associations

Rating

VLA observation of NVSS J191656+051126 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 VLA observation of NVSS J191656+051126, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VLA observation of NVSS J191656+051126 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1081313