HOPS - the H2O southern galactic Plane Survey

Details HOPS - the H2O southern galactic Plane Survey HOPS - the H2O southern galactic Plane Survey

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atnf.prop.2913w&link_type=abstract

ATNF proposal M207, Semester: April, 2010

Computer Science

Masers (Galactic And Extragalactic), Star Formation, Interstellar Medium In And Around The Milky Way, Mopra

Scientific paper

The H2O southern galactic Plane Survey (HOPS) is a 12mm line survey with the Mopra radiotelescope. It will cover 90 square degrees of the Galaxy between l=300 - 0 - 30 degrees and |b|<0.5 degrees. The main spectral lines covered (in order of importance) are: water masers; ammonia (1,1), (2,2), (3,3), (6,6) and (9,9); cyanoacetylene (HCCCN); methanol (both masing and thermal) and radio recombination lines. Such a survey will complement the methanol multibeam survey, and lead to a bettter understanding of the connection between water and methanol masers. It will also identify many previously unknown sites of star formation in our Galaxy through ammonia and cyanoacetylene emission. This will lead to a more complete picture of star formation throughout the southern Galaxy. We ask for a further 105 hours (7x15hour days) to finish the Mopra part of HOPS.

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