A new weak OH maser source near the post-AGB star OH 17.7-2.0.

Details A new weak OH maser source near the post-AGB star OH 17.7-2.0. A new weak OH maser source near the post-AGB star OH 17.7-2.0.

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998acaps..18..419y&link_type=abstract

Acta Astrophys. Sin., Vol. 18, No. 4, p. 419 - 422

Astronomy and Astrophysics

Astrophysics

Post-Agb Stars: Oh Masers

Scientific paper

The authors have observed the weak OH maser source near OH 17.7-2.0 using the Parkes 64 m radio telescope, Australia. The OH maser emission was observed at five different locations. The observations indicate that a new weak OH maser source, with peak velocity at 53.5 km/s, has been found. The best-fitting position of this new OH maser source has been determined using a two-dimensional Gaussian fitting procedure.

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