H2O masers in the direction of southern nebular objects

Details H2O masers in the direction of southern nebular objects H2O masers in the direction of southern nebular objects

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...104..166s&link_type=abstract

Astronomy and Astrophysics, vol. 104, no. 1, Dec. 1981, p. 166-168. Research supported by the Financiadora de Estudos e Projeto

Astronomy and Astrophysics

Astronomy

10

Interstellar Masers, Nebulae, Orion Constellation, Southern Sky, T Tauri Stars, Water Masers, Cosmic Dust, Emission Spectra, Infrared Stars, Radio Astronomy, Stellar Envelopes, Stellar Luminosity

Scientific paper

Thirteen Orion population stars and 4 H-H objects were searched for water maser emission. Two variable water masers were detected toward RU Lupi and vBH 656, which represent the first southern water masers associated with low luminosity stars. Both masers are very weak, and their accurate positions have not been determined, thus it is not known whether the masers originate in the dust envelopes surrounding the two T Tauri stars.

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