Mapping the great attractor region in X rays and diffuse X ray emission: A possible galactic wind in the bulge of M31

Details Mapping the great attractor region in X rays and diffuse X ray emission: A possible galactic wind in the bulge of M31 Mapping the great attractor region in X rays and diffuse X ray emission: A possible galactic wind in the bulge of M31

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sao..rept.....f&link_type=abstract

Final Report, 1 Aug. 1989 - 31 Jul. 1991 Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astrophysics

Galactic Bulge, Galactic Clusters, X Rays, Andromeda Galaxy, Astronomical Catalogs, Computer Programs, Data Processing, Interstellar Gas, Stellar Luminosity

Scientific paper

The NASA ADP Program to study the x ray emission in the direction of the
Great Attractor and from the core of M31 has resulted in four papers;
three on the Shapley Supercluster which is the dominant x ray feature in
the Great Attractor region and one on the diffuse emission in M31. The
results of these papers are summarized.

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