Radio Sources in the Vicinity of Source M 31
The region α (right ascension) equal to 23$^{h}$ 50$^{m}$ to 01$^{h}$ 30$^{m}$, δ (declination) 39° 20′ to 40 degrees 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...
Saved in:
Published in: | Science (American Association for the Advancement of Science) Vol. 158; no. 3804; pp. 1043 - 1045 |
---|---|
Main Author: | |
Format: | Journal Article |
Language: | English |
Published: |
United States
American Association for the Advancement of Science
24-11-1967
|
Subjects: | |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Summary: | The region α (right ascension) equal to 23$^{h}$ 50$^{m}$ to 01$^{h}$ 30$^{m}$, δ (declination) 39° 20′ to 40 degrees 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. |
---|---|
Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0036-8075 1095-9203 |
DOI: | 10.1126/science.158.3804.1043 |