High-resolution observations of ionized gas in central 3 parsecs of the Galaxy - Possible evidence for infall

Details High-resolution observations of ionized gas in central 3 parsecs of the Galaxy - Possible evidence for infall High-resolution observations of ionized gas in central 3 parsecs of the Galaxy - Possible evidence for infall

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983natur.306..647l&link_type=abstract

Nature (ISSN 0028-0836), vol. 306, Dec. 15, 1983, p. 647-651.

Astronomy and Astrophysics

Astronomy

147

Galactic Nuclei, Gravitational Effects, Interstellar Gas, Ionized Gases, Milky Way Galaxy, Astronomical Maps, Astronomical Models, Gas Streams, High Resolution, Nebulae

Scientific paper

A 1 arcsec resolution radio map shows a wealth of detail in the "spiral" distribution of ionized gas within 1.5 pc of the galactic centre. Three streams of ionized gas passing near the centre can be identified. These streams could be due to molecular gas falling in towards the centre, in which case one has the first direct observation of the paths of accretion by a galactic nucleus.

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