A search for hydroxyl masers in M33

Details A search for hydroxyl masers in M33 A search for hydroxyl masers in M33

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aj.....90..736f&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 90, May 1985, p. 736, 737.

Astronomy and Astrophysics

Astronomy

2

Galactic Structure, Hydroxyl Emission, Interstellar Masers, Spiral Galaxies, Stellar Luminosity, Circular Polarization, Ground State, Hot Stars, Magellanic Clouds, Molecular Clouds, Spatial Distribution, Stellar Evolution, Very Large Array (Vla)

Scientific paper

The authors have used the NRAO Very Large Array to search for emission
from the 2π3/2 ground-state transitions of
hydroxyl in the direction of the nearby Sc galaxy M33. They detected no
hydroxyl masers and conclude that there are no type I masers in M33 that
are as luminous as the brightest type I masers in our galaxy.

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