Periodic flares in the methanol maser source G9.62+0.20E

Details Periodic flares in the methanol maser source G9.62+0.20E Periodic flares in the methanol maser source G9.62+0.20E

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mnras.339l..33g&link_type=abstract

Monthly Notice of the Royal Astronomical Society, Volume 339, Issue 4, pp. L33-L36.

Astronomy and Astrophysics

Astronomy

21

Masers, Stars: Formation, Ism: Clouds, Hii Regions, Radio Lines: Ism

Scientific paper

The class II methanol maser source G9.62+0.20E has been monitored since
1999 at 6.7 GHz and since 2000 at 12.2 GHz. Six flares have been
observed to date. These flares are periodic, with an interval of 246 d
between flares. The duration of the flare is approximately 3 months,
with maximum amplitude reached a month after the start of the flare.

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