A 330 MHz Survey for Pulsars and Supernova Remnants in M31

Details A 330 MHz Survey for Pulsars and Supernova Remnants in M31 A 330 MHz Survey for Pulsars and Supernova Remnants in M31

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xrrc.proce4.10g&link_type=abstract

"X-Ray and Radio Connections (eds. L.O. Sjouwerman and K.K Dyer) Published electronically by NRAO, http://www.aoc.nrao.edu/event

Physics

X-Ray, Radio, Supernova Remnants

Scientific paper

In the radio band, supernova remnants (SNR) and pulsars are best identified at low frequencies due to their steep spectra. Motivated by this fact, we have carried out a deep 330 MHz observation of M31 using the VLA. Achieving a sensitivity of 0.6 mJy at 6 arcsec resolution over the entire optical disk of M31, we identified 405 distinct radio sources. While most of these are unresolved background radio galaxies, we found five SNR candidates, three pulsar wind nebula (PWN) candidates, and three pulsar candidates in our source list. The properties of these sources are discussed.

Affiliated with

Also associated with

No associations

Rating

A 330 MHz Survey for Pulsars and Supernova Remnants in M31 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 A 330 MHz Survey for Pulsars and Supernova Remnants in M31, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A 330 MHz Survey for Pulsars and Supernova Remnants in M31 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1555638