Global Studies of Molecular Clouds in the Galaxy, The Magellanic Clouds, and M31

Details Global Studies of Molecular Clouds in the Galaxy, The Magellanic Clouds, and M31 Global Studies of Molecular Clouds in the Galaxy, The Magellanic Clouds, and M31

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999stin...0011950t&link_type=abstract

Technical Report, Smithsonian Astrophysical Observatory Cambridge, MA United States

Astronomy and Astrophysics

Astrophysics

Andromeda Galaxy, Magellanic Clouds, Molecular Clouds, Gamma Ray Astronomy, Astrophysics, Galactic Mass, X Ray Sources, Point Sources, Rosat Mission, Cosmic Background Explorer Satellite, Infrared Astronomy Satellite, Mass Distribution, H Ii Regions

Scientific paper

Over the course of this grant we used various spacecraft surveys of the Galaxy and M31 in conjunction with our extensive CO spectral line surveys to address central problems in galactic structure and the astrophysics of molecular clouds. These problems included the nature of the molecular ring and its relation to the spiral arms and central bar, the cosmic ray distribution, the origin of the diffuse X-ray background, the distribution and properties of x-ray sources and supernova remnants, and the Galactic stellar mass distribution. For many of these problems, the nearby spiral M31 provided an important complementary perspective. Our CO surveys of GMCs (Galactic Molecular Clouds) were crucial for interpreting Galactic continuum surveys from satellites such as GRO (Gamma Ray Observatory), ROSAT (Roentgen Satellite), IRAS (Infrared Astronomy Satellite), and COBE (Cosmic Background Explorer Satellite) because they provided the missing dimension of velocity or kinematic distance. GMCs are a well-defined and widespread population of objects whose velocities we could readily measure throughout the Galaxy. Through various emission and absorption mechanisms involving their gas, dust, or associated Population I objects, GMCs modulate the galactic emission in virtually every major wavelength band. Furthermore, the visibility. of GMCs at so many wavelengths provided various methods of resolving the kinematic distance ambiguity for these objects in the inner Galaxy. Summaries of our accomplishments in each of the major wavelength bands discussed in our original proposal are given

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