The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratios

G. J. Bendo; M. Baes; S. Bianchi; M. Boquien; A. Boselli; A. Cooray; L. Cortese; I. De Looze; S. Di Serego Alighieri; J. Fritz; G. Gentile; T. M. Hughes; N. Lu; C. Pappalardo; M. W. L. Smith; L. Spinoglio; S. Viaene; C. Vlahakis

doi:10.1093/mnras/stu1841

The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratios

G. J. Bendo, M. Baes, S. Bianchi, M. Boquien, A. Boselli, A. Cooray, L. Cortese, I. De Looze, S. Di Serego Alighieri, J. Fritz, G. Gentile, T. M. Hughes, N. Lu, C. Pappalardo, M. W. L. Smith, L. Spinoglio, S. Viaene, C. Vlahakis

Research output: Contribution to journal › Article › peer-review

Abstract

We examined variations in the 160/250 and 250/350 μm surface brightness ratios within 24 nearby (

Original language	English
Pages (from-to)	135-167
Number of pages	32
Journal	Royal Astronomical Society. Monthly Notices
Volume	448
Issue number	1
DOIs	https://doi.org/10.1093/mnras/stu1841
Publication status	Published - Mar 2015

Keywords

galaxies: ISM
galaxies: spiral
infrared: galaxies

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10.1093/mnras/stu1841

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Bendo, G. J., Baes, M., Bianchi, S., Boquien, M., Boselli, A., Cooray, A., Cortese, L., De Looze, I., Di Serego Alighieri, S., Fritz, J., Gentile, G., Hughes, T. M., Lu, N., Pappalardo, C., Smith, M. W. L., Spinoglio, L., Viaene, S., & Vlahakis, C. (2015). The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratios. Royal Astronomical Society. Monthly Notices, 448(1), 135-167. https://doi.org/10.1093/mnras/stu1841

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title = "The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratios",

abstract = "We examined variations in the 160/250 and 250/350 μm surface brightness ratios within 24 nearby (",

keywords = "galaxies: ISM, galaxies: spiral, infrared: galaxies",

author = "Bendo, {G. J.} and M. Baes and S. Bianchi and M. Boquien and A. Boselli and A. Cooray and L. Cortese and {De Looze}, I. and {Di Serego Alighieri}, S. and J. Fritz and G. Gentile and Hughes, {T. M.} and N. Lu and C. Pappalardo and Smith, {M. W. L.} and L. Spinoglio and S. Viaene and C. Vlahakis",

year = "2015",

month = mar,

doi = "10.1093/mnras/stu1841",

language = "English",

volume = "448",

pages = "135--167",

journal = "Royal Astronomical Society. Monthly Notices",

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Bendo, GJ, Baes, M, Bianchi, S, Boquien, M, Boselli, A, Cooray, A, Cortese, L, De Looze, I, Di Serego Alighieri, S, Fritz, J, Gentile, G, Hughes, TM, Lu, N, Pappalardo, C, Smith, MWL, Spinoglio, L, Viaene, S & Vlahakis, C 2015, 'The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratios', Royal Astronomical Society. Monthly Notices, vol. 448, no. 1, pp. 135-167. https://doi.org/10.1093/mnras/stu1841

TY - JOUR

T1 - The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratios

AU - Bendo, G. J.

AU - Baes, M.

AU - Bianchi, S.

AU - Boquien, M.

AU - Boselli, A.

AU - Cooray, A.

AU - Cortese, L.

AU - De Looze, I.

AU - Di Serego Alighieri, S.

AU - Fritz, J.

AU - Gentile, G.

AU - Hughes, T. M.

AU - Lu, N.

AU - Pappalardo, C.

AU - Smith, M. W. L.

AU - Spinoglio, L.

AU - Viaene, S.

AU - Vlahakis, C.

PY - 2015/3

Y1 - 2015/3

N2 - We examined variations in the 160/250 and 250/350 μm surface brightness ratios within 24 nearby (

AB - We examined variations in the 160/250 and 250/350 μm surface brightness ratios within 24 nearby (

KW - galaxies: ISM

KW - galaxies: spiral

KW - infrared: galaxies

U2 - 10.1093/mnras/stu1841

DO - 10.1093/mnras/stu1841

M3 - Article

SN - 1365-2966

VL - 448

SP - 135

EP - 167

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

IS - 1

ER -

The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratios

Abstract

Keywords

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