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Publication Details
AFRICAN RESEARCH NEXUS
SHINING A SPOTLIGHT ON AFRICAN RESEARCH
general
Is the bulge of our Galaxy triaxial?
Nature, Volume 353, No. 6340, Year 1991
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Description
AS in the case of other spiral galaxies, such as M31 (refs 1, 2), the rotation curve of gas in our Galaxy indicates that its nuclear bulge is triaxial3. Despite several studies4,5 of the distribution of specific objects in the galactic bulge, no observational evidence of asymmetry has emerged. Recently, however, Blitz and Spergel6 have reanalysed balloon-infrared observations at 2.4 μm, where obscuration is relatively low, to suggest that the galactic bulge is bar-like, and tilted with respect to the plane of the Galaxy. Here we report that the distribution of IRAS (the Infrared Astronomy Satellite) bulge stars shows an asymmetry with respect to the Galactic Centre, providing clear evidence for triaxiality. © 1991 Nature Publishing Group.
Authors & Co-Authors
Nakada, Yoshikazu
Japan, Tokyo
The University of Tokyo
Degucji, S.
Japan, Mitaka
National Institutes of Natural Sciences - National Astronomical Observatory of Japan
Hashimoto, Osamu
Japan, Musashino
Seikei University
Izumiura, Hideyuki
Japan, Koganei
Tokyo Gakugei University
Onaka, Takahashi
Japan, Tokyo
The University of Tokyo
Sekiguchi, Kazuhiro
South Africa, Cape Town
South African Astronomical Observatory
Yamamura, Issei
Japan, Tokyo
The University of Tokyo
Statistics
Citations: 73
Authors: 7
Affiliations: 5
Identifiers
Doi:
10.1038/353140a0
ISSN:
00280836
Research Areas
Cancer