The H2O/OH maser 342.01+0.25 - A case of supernova-induced star formation?

Details The H2O/OH maser 342.01+0.25 - A case of supernova-induced star formation? The H2O/OH maser 342.01+0.25 - A case of supernova-induced star formation?

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...124..139s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 124, no. 1, July 1983, p. 139-142. Research supported by the Financiadora de E

Astronomy and Astrophysics

Astrophysics

1

Hydroxyl Emission, Interstellar Masers, Late Stars, Star Formation, Supernova Remnants, Water Masers, Infrared Radiation, Molecular Spectra

Scientific paper

Time variable H2O emission toward the 1612/1667 MHz OH maser OH 342.01+0.25 has been detected. The maser is seen in the direction of a windswept dark nebula interacting with the supernova remnant Kes 45. The maser has no optical counterpart, although it is a rather bright object in the IR (L = 2.83). The rapid temporal variations of the H2O maser suggest that the maser is associated with a young object and not a late type star. Possibly the H2O/1667 MHz OH maser originates in an object not associated with the 1612 MHz OH/IR source. If the H2O maser is young, the close association with Kes 45 may represent an example of supernova-induced star formation.

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