Artigo Revisado por pares

Carbon monoxide in the inner Galaxy - The 3 kiloparsec arm and other expanding features

1980; IOP Publishing; Volume: 242; Linguagem: Inglês

10.1086/158446

ISSN

1538-4357

Autores

T. M. Bania,

Tópico(s)

Gamma-ray bursts and supernovae

Resumo

view Abstract Citations (77) References (27) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Carbon monoxide in the inner Galaxy - The 3 kiloparsec arm and other expanding features Bania, T. M. Abstract A survey of the latitude distribution of (C-12)O emission in the inner Galaxy shows that much of the dense molecular gas is found in several large-scale features spanning tens of degrees in l. The most prominent are the rotating nuclear disk, the 3 kpc arm, and the +135 km/s features. Each of these features is moving with a high (50-180 km/s) noncircular velocity, which can be unambiguously interpreted as expansion away from the galactic center. The (l, v) loci of the 3 kpc arm and +135 km/s feature can be described by simple kinematic ring structures, but the same ring cannot account for both objects. Publication: The Astrophysical Journal Pub Date: November 1980 DOI: 10.1086/158446 Bibcode: 1980ApJ...242...95B Keywords: Carbon Monoxide; Galactic Structure; Milky Way Galaxy; Molecular Clouds; Astronomical Maps; Explosions; Galactic Nuclei; Gas Expansion; H Lines; Astrophysics full text sources ADS |

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