Duplicity of the 'supermassive' object R136a

Details Duplicity of the 'supermassive' object R136a Duplicity of the 'supermassive' object R136a

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...278l.109w&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 278, March 15, 1984, p. L109.

Astronomy and Astrophysics

Astrophysics

7

Binary Stars, Nebulae, Supermassive Stars, Visual Observation, Magellanic Clouds, Stellar Mass

Scientific paper

It is pointed out that the present controversy over the nature of R136a,
concerning whether it is a single supermassive object or a cluster of
stars, is largely answered by the observations of Innes (1927) and the
comment of van den Bos (1928). It is a nebulous double star with a
position angle of about 220 deg and a separation of 0.5 arcsec.

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