Spectra of Star Formation Regions at the 6.7 GHz Methanol Line

Details Spectra of Star Formation Regions at the 6.7 GHz Methanol Line Spectra of Star Formation Regions at the 6.7 GHz Methanol Line

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aj....127.3479g&link_type=abstract

The Astronomical Journal, Volume 127, Issue 6, pp. 3479-3483.

Astronomy and Astrophysics

Astronomy

3

Radio Lines: General, Stars: Formation

Scientific paper

Seven star formation regions have been observed in the 51-->60A+ transition of the methanol molecule over a 9 month period beginning in 1994 June. Measurements were made with the Penticton 25.6 m paraboloid and a correlation spectrometer. Since these observations were taken several years before publication of spectra from other northern hemisphere observatories, they provide earlier epoch examples for the study of variability. The major feature in one region appeared to have increased by about 10% in 2 days.

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