Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.


Science 24 November 1967:
Vol. 158. no. 3804, pp. 1043 - 1045
DOI: 10.1126/science.158.3804.1043

Articles

Radio Sources in the Vicinity of Source M 31

Carlos M. Varsavsky 1

1 Instituto Argentino de Radioastronomía, Villa Elisa, Pcia. de Buenos Aires, and Arecibo Ionospheric Observatory, Arecibo, Puerto Rico

The region agr (right ascension) equal to 23h 50m to 01h 30m, dgr (declination) 39°20' to 40°40' has been observed at 195 and 430 megahertz with the 1000-foot (300 m) telescope of the Arecibo Ionospheric Observatory. Eighteen sources from the Ohio Catalogue and source 3C 13 are contained in this region. We conclude that the sources have straight-line spectra with indices between -0.4 and -0.9 and that they are probably not associated with M 31, except those within the optical limit of the nebula.





To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)