Monitoring of 6-cm excited OH masers - II

Details Monitoring of 6-cm excited OH masers - II Monitoring of 6-cm excited OH masers - II

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mnras.339....1s&link_type=abstract

Monthly Notice of the Royal Astronomical Society, Volume 339, Issue 1, pp. 1-11.

Astronomy and Astrophysics

Astronomy

12

Masers, Stars: Formation, Ism: Molecules, Radio Lines: Ism

Scientific paper

A search towards 69 star-forming regions has led to the discovery of three new 4765-MHz excited OH masers. No 4750- or 4660-MHz excited OH masers were detected above a level of ~1 Jy. The results of monitoring nine sources of 4765-MHz excited OH masers for periods of up to 7 yr are reported. Many of the linewidths are narrow and have had constant widths and centroid velocities throughout the monitoring period. The maser flux of one source was constant over 7 yr while in the most extreme case of variability the flux doubled in a period of 2 weeks.

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