Westerbork and VLA observations of G 127.1+0.5

Details Westerbork and VLA observations of G 127.1+0.5 Westerbork and VLA observations of G 127.1+0.5

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...112..120p&link_type=abstract

Astronomy and Astrophysics, vol. 112, no. 1, Aug. 1982, p. 120-123.

Astronomy and Astrophysics

Astronomy

11

Point Sources, Radio Sources (Astronomy), Star Clusters, Supernova Remnants, Absorption Spectra, Astronomical Maps, Open Clusters, Radio Telescopes, Very Large Array (Vla)

Scientific paper

The Galactic supernova remnant (SNR) G 127.1+0.5 contains the open cluster NGC 559 and the radio point source 0125+628 within its boundaries. Continuum measurements of the SNR at 608.5 MHz with the Westerbork Synthesis Radio Telescope (WSRT), and H I absorption spectra toward 0125+628 with the WSRT and the Very Large Array (VLA) are reported. The observations strongly suggest that there is no physical connection between the SNR, the point source, and the open cluster.

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