High dynamic-range observations of the supernova remnant G 39.2 - 0.3 and the H II region NRAO 591

Details High dynamic-range observations of the supernova remnant G 39.2 - 0.3 and the H II region NRAO 591 High dynamic-range observations of the supernova remnant G 39.2 - 0.3 and the H II region NRAO 591

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...232..467p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 232, no. 2, June 1990, p. 467-476.

Astronomy and Astrophysics

Astrophysics

11

H Ii Regions, Supernova Remnants, Emissivity, Interstellar Magnetic Fields, Polarized Radiation, Stellar Envelopes, Very Large Array (Vla)

Scientific paper

Radio observations of the SNR G 39.2 - 0.3 (obtained with the VLA at 1.5 and 5 GHz and with the OSRT at 327 MHz) and of the H II complex NRAO 591 (obtained with the VLA at 327 MHz and 1.5 GHz) are reported. The data are presented in tables, graphs, and contour maps and characterized in detail. It is found that the emission near the SNR shell is highly nonuniform, with a flat spectrum and a tail extending for about 135 deg in a curve to the east of the SNR. The distance to NRAO 591 is estimated as 14 kpc, and a partial shell structure is detected in the compact 'head' region.

Affiliated with

Also associated with

No associations

Rating

High dynamic-range observations of the supernova remnant G 39.2 - 0.3 and the H II region NRAO 591 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 High dynamic-range observations of the supernova remnant G 39.2 - 0.3 and the H II region NRAO 591, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High dynamic-range observations of the supernova remnant G 39.2 - 0.3 and the H II region NRAO 591 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-980856