VLA observations of the fast pulsar candidate in M 28

Details VLA observations of the fast pulsar candidate in M 28 VLA observations of the fast pulsar candidate in M 28

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...314l..45e&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 314, March 15, 1987, p. L45-L47.

Astronomy and Astrophysics

Astronomy

9

Globular Clusters, Pulsars, Radio Sources (Astronomy), Radio Spectra, Stellar Evolution

Scientific paper

The radio source at the center of the globular cluster M 28 is observed with the VLA at 327 MHz, confirming previous lower-frequency observations (Mahoney and Erickson, 1985) which indicated that this source has an unusually steep spectrum. It appears to be compact, and it is also highly polarized, giving it a set of properties characteristic of radio pulsars. Evolutionary considerations, along with its nondetection in previous pulsar surveys, strongly suggest that it is a millisecond pulsar.

Affiliated with

Also associated with

No associations

Rating

VLA observations of the fast pulsar candidate in M 28 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 observations of the fast pulsar candidate in M 28, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VLA observations of the fast pulsar candidate in M 28 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1452964