Radio emission from stars projected on the galactic cluster A3487

Details Radio emission from stars projected on the galactic cluster A3487 Radio emission from stars projected on the galactic cluster A3487

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ap.....54..371l&link_type=abstract

Astrophysics, Volume 54, Issue 3, pp.371-376

Astronomy and Astrophysics

Astrophysics

Stars, Radio Sources, Optical Identifications

Scientific paper

Radio stars are identified optically with bright stars located in the direction of the cluster A3487 (RA(J) = 11h31m58s, DEC(J) = -31°11'34".8) with an accuracy determined by the refraction of radio waves in the interstellar medium in this direction of the sky. Within an area of 1 sq. degree, 60% of the strong radio sources with P > 0.004 Jy are identified with stars brighter than 10 m.

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