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Sökning: id:"swepub:oai:research.chalmers.se:c1c1b51d-472f-4971-9432-2d6e0e91ea37" > Physical properties...

Physical properties of outflows Comparing CO- and H2O-based parameters in Class 0 sources

Bjerkeli, Per, 1977 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
Liseau, René, 1949 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
Nisini, B. (författare)
Osservatorio Astronomico di Roma
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Tafalla, M. (författare)
Observatorio Astronómico Nacional (OAN),Spanish National Observatory (OAN)
Bergman, Per, 1960 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
Melnick, G. J. (författare)
Harvard-Smithsonian Center for Astrophysics
Rydbeck, Gustaf, 1942 (författare)
Chalmers tekniska högskola,Chalmers University of Technology
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 (creator_code:org_t)
2013-03-29
2013
Engelska.
Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 552
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
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  • Context. The observed physical properties of outflows from low-mass sources put constraints on possible ejection mechanisms. Historically, these quantities have been derived from CO using ground-based observations. It is, therefore, important to investigate whether parameters such as momentum rate (thrust) and mechanical luminosity (power) are the same when different molecular tracers are used.Aims. Our objective is to determine the outflow momentum, dynamical time-scale, thrust, energy, and power using CO and H2O as tracers of outflow activity.Methods. Within the framework of the Water In Star-forming regions with Herschel (WISH) key program, three molecular outflows from Class 0 sources have been mapped using the Heterodyne Instrument for the Far Infrared (HIFI) instrument aboard Herschel. We used these observations together with previously published H-2 data to infer the physical properties of the outflows. We compared the physical properties derived here with previous estimates based on CO observations.Results. Inspection of the spatial distribution of H2O and H-2 confirms that these molecules are co-spatial. The most prominent emission peaks in H-2 coincide with strong H2O emission peaks and the estimated widths of the flows when using the two tracers are comparable.Conclusions. For the momentum rate and the mechanical luminosity, inferred values are not dependent on which tracer is used, i.e. the values agree to within a factor of 4 and 3, respectively.

Ämnesord

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

Nyckelord

hifi
stars: formation
shock-waves
protostellar outflows
bipolar outflow
water emission
ISM: jets and outflows
herschel-pacs
h-2 emission
l1157
stars: winds
star-forming regions
ISM: molecules
driven molecular outflows
outflows

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art (ämneskategori)
ref (ämneskategori)

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