Is HD26676 an unusual radio star

Details Is HD26676 an unusual radio star Is HD26676 an unusual radio star

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978natur.274..137p&link_type=abstract

Nature, vol. 274, July 13, 1978, p. 137. NSF-supported research.

Astronomy and Astrophysics

Astronomy

2

B Stars, Late Stars, Radial Velocity, Radio Sources (Astronomy), Radio Stars, Balmer Series, Binary Stars

Scientific paper

A high-dispersion search for radial velocity variations in HD 26676 suggests that it is unlikely that this 6 mag late B star is a close binary. This conclusion is of interest because a faint radio source has been found to have a position coincident with this star, and all previously identified radio stars are radio and optical variables and/or binaries. Thus it is possible that the object may represent a new class of radio star. The treatment of the radial velocity data is described, the existence of a prominent reflection nebula surrounding the star is noted, and the reduction of the size of the radio error box is considered.

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