Observation of methanol maser sources with the Arcetri 12 GHz receiver

Details Observation of methanol maser sources with the Arcetri 12 GHz receiver Observation of methanol maser sources with the Arcetri 12 GHz receiver

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...98..127c&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 98, no. 1, p. 127-135.

Astronomy and Astrophysics

Astrophysics

5

Interstellar Masers, Line Spectra, Methyl Alcohol, Astronomical Spectroscopy, Emission Spectra, Radio Telescopes, Stellar Envelopes

Scientific paper

A 12.2 GHz receiver has been designed and built to observe the 2(0) -
3(-1) E methanol transition. Laboratory tests and first spectral
observations show that its stability and sensitivity are satisfactory.
The observations point out the time stability of methanol maser sources
on a time scale of the order of 2-8 months.

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