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Ionized gas in the Sgr A complex -- VLA observations of H168α and H270α recombination lines

dc.additional1999 Astronomical Society of the Pacificen
dc.contributor.authorAnantharamaiah, K R
dc.contributor.authorPedlar, A
dc.contributor.authorGoss, W M
dc.date.accessioned2007-05-25T09:28:23Z
dc.date.available2007-05-25T09:28:23Z
dc.date.issued1999
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations).en
dc.description.abstractRadio recombination lines at λ = 20 cm reveal the presence of an extended component of ionized gas of lower density (~100 cm3) in the Sgr A complex. This component extends well beyond the thermal `mini-spiral' Sgr A-West which seem to be embedded in it. The low-density component is present over the entire extent of Sgr A East and possibly beyond and it is responsible for the turnover in the spectrum of Sgr A East and the halo observed by Pedlar et al (1989) at λ = 90 cm. The radial velocity of the extended ionized gas ranges from +50 kms- to --200 kms- with minima of emission near --50 and --150 kms. The total mass of the low-density component is estimated to be ~104 Modot. A possible extended feature at a high velocity of 470 kms- is also detected, but needs further observations to confirm it.en
dc.format.extent993912 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationASP Conference Series, 1999, Vol.186, p422en
dc.identifier.isbn1-58381-012-9
dc.identifier.urihttp://hdl.handle.net/2289/2457
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1999ASPC..186..422Aen
dc.relation.urihttp://arxiv.org/abs/astro-ph/9903072en
dc.rightsThe Central Parsecs of the Galaxy, ASP Conference Series, Vol. 186. Eds. Heino Falcke, Angela Cotera, Wolfgang J. Duschl, Fulvio Melia, and Marcia J. Rieke, 1999.en
dc.titleIonized gas in the Sgr A complex -- VLA observations of H168α and H270α recombination linesen
dc.typeArticleen

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