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2011MNRAS.416....2H - Mon. Not. R. Astron. Soc., 416, 2-12 (2011/September-1)
Atomic hydrogen produced in M33 photodissociation regions.
HEINER J.S., ALLEN R.J. and VAN DER KRUIT P.C.
Abstract (from CDS):
We describe our `PDR method' in more detail and apply it using GALEX FUV and Very Large Array 21-cm radio data to obtain volume densities in a selection of GMCs in the nearby spiral galaxy M33. We have also examined the sensitivity of the method to the linear resolution of the observations used; the results obtained at 20 pc are similar to those for the larger set of data at 80-pc resolution. The cloud densities we derive range from 1 to 500/cm3, with no clear dependence on the galactocentric radius; these results are generally similar to those obtained earlier in the cases of M81, M83 and M101 using the same method. Herschel-ATLAS: the link between accretion luminosity and star formation in quasar host galaxies
Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS
Journal keyword(s): ISM: atoms - ISM: clouds - ISM: molecules - galaxies: individual: M33 - galaxies: ISM - ultraviolet: galaxies
VizieR on-line data: <Available at CDS (J/MNRAS/416/2): table5.dat table6.dat>
Nomenclature: Table 3: [HAV2011] Region 42 N=1. Table 5: [HAV2011] NN (Nos 1-42). Table 6: [HAV2011] NNa N=208.
Status at CDS : All or part of tables of objects could be ingested in SIMBAD with priority 2.
Simbad objects: 16
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