1994
DOI: 10.1086/117188
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Two views of the Andromeda Galaxy H-alpha and far infrared

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Cited by 77 publications
(125 citation statements)
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“…Haas et al 1998;Gordon et al 2006), the dust emission in the 1.5 kpc ring region is dominated by a higher temperature component. This is also consistent with the study by Devereux et al (1994), who find that the gas in the innermost regions is dominated by an ionized component (seen in Hα emission). On the other hand, if we only consider the emission from the 10 kpc ring (sampled by our third annulus), we obtain an average temperature of 17.0 +0.3 −0.3 K, and a dust mass of 1.95 × 10 7 M .…”
Section: Dust Masses and Temperaturessupporting
confidence: 93%
See 1 more Smart Citation
“…Haas et al 1998;Gordon et al 2006), the dust emission in the 1.5 kpc ring region is dominated by a higher temperature component. This is also consistent with the study by Devereux et al (1994), who find that the gas in the innermost regions is dominated by an ionized component (seen in Hα emission). On the other hand, if we only consider the emission from the 10 kpc ring (sampled by our third annulus), we obtain an average temperature of 17.0 +0.3 −0.3 K, and a dust mass of 1.95 × 10 7 M .…”
Section: Dust Masses and Temperaturessupporting
confidence: 93%
“…(Pietsch et al 2005), ultraviolet , optical (e.g. SDSS, Hα by Devereux et al 1994; or the PAndAS survey, see e.g. McConnachie et al 2008), near and far-infrared (FIR) (Haas et al 1998;Barmby et al 2006;Gordon et al 2006;Beaton et al 2007;Krause et al, in prep.…”
Section: Introduction An Overall View Of the Interstellar Medium Of Tmentioning
confidence: 99%
“…Of course, the current SFR value can also be used directly. The SFR estimates for M 31 are in the range ≈0.4-0.8 M yr −1 (Barmby et al 2006;Devereux et al 1994), and with the Sullivan et al (2006) calibration, we obtain an SN Ia rate of (0.5-0.6) × 10 −3 SNe yr −1 per 10 10 M , also compatible with the above numbers.…”
Section: Sn Ia Rate In M 31supporting
confidence: 88%
“…(1) Beck et al (1998); (2) Tabatabaei et al (2007b); (3) Gordon et al (2006); (4) Tabatabaei et al (2007a); (5) Devereux et al (1994); (6) Hoopes & Walterbos (2000).…”
Section: Introductionmentioning
confidence: 99%
“…This is due to the synchrotron emission being underestimated when the nonthermal spectral index is flatter than the one assumed in the standard method. Possible origins of the strong Hα emission and high thermal fraction at R < 30 have been discussed by Devereux et al (1994) and Tabatabaei & Berkhuijsen (2010). As recent SF is scarce in this region, the gas must have been ionized by shocks, evolved stars (Groves et al 2012) and/or during the last encounter with a companion galaxy (Block et al 2006).…”
mentioning
confidence: 99%