Radio Morphologies and Spectra of Compact Radio Sources with the Steepest Spectra

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5

Catalogs, Galaxies: Active, Stars: Pulsars: General, Radio Continuum: Galaxies, Radio Continuum: Stars, Surveys

Scientific paper

We have assembled a complete sample of 74 compact (θ<=25'') radio sources visible from the northern hemisphere with spectral indexes 1.5<=α<=3.2 (where Sν~ν-α) and 365 MHz flux densities S>=200 mJy. These sources were selected from two large-scale radio surveys: the 1.4 GHz NRAO VLA Sky Survey and the 365 MHz Texas survey, which together cover almost 80% of the sky (- 35deg30'<=δ<=71deg30'). We present here high-resolution images for the sources and spectra compiled from our data and other surveys. We attempt to classify these sources based on morphology and size determined by additional radio observations using the Very Large Array. We cannot definitively classify the majority of the sources based on these data, but statistical arguments suggest most are distant radio galaxies. A small number of previously unknown pulsars may also exist in our sample.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Radio Morphologies and Spectra of Compact Radio Sources with the Steepest Spectra 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 Radio Morphologies and Spectra of Compact Radio Sources with the Steepest Spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio Morphologies and Spectra of Compact Radio Sources with the Steepest Spectra will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1253367

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.