SIMBAD references

2002A&A...385.1049T - Astronomy and Astrophysics, volume 385, 1049-1055 (2002/4-3)

Water maser emission in IC 342.

TARCHI A., HENKEL C., PECK A.B. and MENTEN K.M.

Abstract (from CDS):

The detection of 22GHz water vapor emission from IC 342 is reported, raising the detection rate among northern galaxies with IRAS point source fluxes S100µm>50Jy to 16%. The maser, associated with a star forming region ∼10-15" west of the nucleus, consists of a single 0.5km/s wide feature and reaches an isotropic luminosity of 10–2L (D=1.8Mpc). If the time variability is intrinsic, the maser size is ≲1.5x1016cm (≲0.5mas) which corresponds to a brightness temperature of >109K. The linewidth, luminosity, and rapid variability are reminiscent of the 8km/s super maser in Orion-KL. A velocity shift of 1km/s within two weeks and subsequent rapid fading is explained in terms of a chance alignment of two dense molecular clouds. Observations at 22GHz toward Maffei 2 are also reported, yielding a 5σ upper limit of 25mJy for a channel spacing of 1.05km/s.

Abstract Copyright:

Journal keyword(s): galaxies: individual: IC 342, Maffei 2 - galaxies: starburst - ISM: molecules - masers - lines: ISM radio

Simbad objects: 30

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2019.12.12-22:23:56

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