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P Cygni Profiles of Molecular Lines Toward Arp 220 Nuclei

Sakamoto, K. (author)
Academia Sinica Taiwan
Aalto, Susanne, 1964 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Wilner, D.J. (author)
Harvard-Smithsonian Center for Astrophysics
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Black, John H, 1949 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Conway, John, 1963 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Costagliola, Francesco, 1981 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Peck, A. B. (author)
Atacama Large Millimeter-submillimeter Array (ALMA)
Spaans, M. (author)
Rijksuniversiteit Groningen,University of Groningen
Wang, Junzhi (author)
Nanjing University
Wiedner, M.C. (author)
Observatoire de Paris,Paris Observatory
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 (creator_code:org_t)
2009
2009
English.
In: Astrophysical Journal Letters. - 2041-8213 .- 2041-8205. ; 700:2, s. L104-L108
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We report ~100 pc (0farcs3) resolution observations of (sub)millimeter HCO+ and CO lines in the ultraluminous infrared galaxy Arp 220. The lines peak at two merger nuclei, with HCO+ being more spatially concentrated than CO. Asymmetric line profiles with blueshifted absorption and redshifted emission are discovered in HCO+(3-2) and (4-3) toward the two nuclei and in CO(3-2) toward one nucleus. We suggest that these P Cygni profiles are due to ~100 km s–1 outward motion of molecular gas from the nuclei. This gas is most likely outflowing from the inner regions of the two nuclear disks rotating around individual nuclei, clearing the shroud around the luminosity sources there.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

galaxies:evolution
galaxies: individual: Arp 220
galaxies: active

Publication and Content Type

art (subject category)
ref (subject category)

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