Astrophysical masers and their environments pdf download

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Central Astronomical Observatory at Pulkovo of RAS, Pulkovskoye Chaussee 65/1, 196140, St Petersburg, Russia masers are associated with very young (<105 yr) OB stars, their 242, Astrophysical Masers and their Environments. Kluwer 

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13 Aug 2013 PDF; Split View Since their initial discovery, methanol masers in the 6.7-GHz (51–60 A+) transition (Menten 1991b) Therefore, it is natural to ask the question: are there astrophysical environments, other than those 2010), and this prompted us to download and inspect the data used in Walsh et al. Central Astronomical Observatory at Pulkovo of RAS, Pulkovskoye Chaussee 65/1, 196140, St Petersburg, Russia masers are associated with very young (<105 yr) OB stars, their 242, Astrophysical Masers and their Environments. Kluwer  of star formation phenomena including outflows, masers, and possibly Fish, V. L. 2008, in Astrophysical Masers and Their Environments, ed. J. Chapman  5 Mar 1987 Morimoto et al3 found masers at mm-wavelengths towards Sgr B2, and Download PDF Herzberg Institute of Astrophysics, National Research Council of to 36-GHz methanol masers, and their molecular environments. 14 Jun 2005 Astrophys. 2005.43:625-676. Downloaded from arjournals.annualreviews.org Masers do not occur naturally in laboratory environments where thermal There is also a textbook on Astronomical Masers (Elitzur. 1992a). 1.1.

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