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TheHerschelSpace Observatory view of dust in M81

Authors :
Marc Sauvage
N. Lu
Pierre Chanial
Walter Kieran Gear
L. Vigroux
Pasquale Panuzzo
M. Symeonidis
Herve Wozniak
Diane Cormier
George J. Bendo
B. O'Halloran
James J. Bock
M. J. Barlow
Werner W. Zeilinger
Jamie Stevens
Mattia Vaccari
E. E. Rigby
Stephane Charlot
Helene Roussel
David L. Clements
Luca Cortese
Naseem Rangwala
T. J. Parkin
Michael Pohlen
N. Castro-Rodriguez
Matthew Joseph Griffin
Matthew Smith
Sacha Hony
S. Sundar
Maud Galametz
Alessandro Boselli
A. Cooray
Gillian S. Wright
Christine D. Wilson
M. Bradford
Haley Louise Gomez
Stephen Anthony Eales
Koryo Okumura
Andreas Papageorgiou
Eli Dwek
Maximilien R. P. Schirm
Laure Ciesla
Kate Gudrun Isaak
Maarten Baes
N. Sacchi
Suzanne C. Madden
L. R. Levenson
Benjamin L. Schulz
Markos Trichas
Seb Oliver
V. Buat
Ismael Perez-Fournon
Mat Page
Jason Glenn
Robbie Richard Auld
D. Elbaz
Frédéric Galliano
L. Spinoglio
A. Rykala
Jonathan Ivor Davies
Laboratoire d'Astrophysique de Marseille (LAM)
Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Institut d'Astrophysique de Paris (IAP)
Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Observatoire astronomique de Strasbourg (ObAS)
Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Source :
ASTRONOMY & ASTROPHYSICS, Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, 2010, 518, ⟨10.1051/0004-6361/201014568⟩
Publication Year :
2010
Publisher :
EDP Sciences, 2010.

Abstract

We use Herschel Space Observatory data to place observational constraints on the peak and Rayleigh-Jeans slope of dust emission observed at 70-500 microns in the nearby spiral galaxy M81. We find that the ratios of wave bands between 160 and 500 microns are primarily dependent on radius but that the ratio of 70 to 160 micron emission shows no clear dependence on surface brightness or radius. These results along with analyses of the spectral energy distributions imply that the 160-500 micron emission traces 15-30 K dust heated by evolved stars in the bulge and disc whereas the 70 micron emission includes dust heated by the active galactic nucleus and young stars in star forming regions.<br />Accepted for A & A Herschel special issue

Details

ISSN :
14320746 and 00046361
Volume :
518
Database :
OpenAIRE
Journal :
Astronomy and Astrophysics
Accession number :
edsair.doi.dedup.....b199a0ed3f1662ea7254e61d73e0060b
Full Text :
https://doi.org/10.1051/0004-6361/201014568