Multifrequency radio continuum observations of extended galactic objects. II - Eleven objects from the 2695 MHz Effelsberg Galactic plane survey

Details Multifrequency radio continuum observations of extended galactic objects. II - Eleven objects from the 2695 MHz Effelsberg Galactic plane survey Multifrequency radio continuum observations of extended galactic objects. II - Eleven objects from the 2695 MHz Effelsberg Galactic plane survey

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...69..403f&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 69, no. 3, June 1987, p. 403-413. Research supported by the

Astronomy and Astrophysics

Astronomy

18

Astronomical Spectroscopy, Continuous Spectra, Milky Way Galaxy, Radio Spectra, Supernova Remnants, H Ii Regions, Infrared Astronomy Satellite, Infrared Spectra, Radio Frequencies, Sky Surveys (Astronomy), Stellar Envelopes

Scientific paper

The 2695-MHz Galactic-plane survey with the Effelsberg 100-m telescope (Reich et al., 1984) has been inspected for shell-type or complex objects, most of which have been formerly unidentified. Eleven objects have additionally been observed at 1420 MHz, 4750 MHz, and 10.55 GHz. The IRAS sky survey was also searched for associated infrared emission. Based on the available data, the most probable identifications of four new shell-type supernova remnants and seven H II regions are proposed. Among the H II regions is a shell of about 30 x 22 pc in extent centered on a B0 star. Another thermal shell surrounds a slightly extended nonthermal source which might be a distant plerionic-type supernova remnant.

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