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Infrared Array Camera (IRAC) Observations of M81

Willner, S. P. and Ashby, M. L. N. and Barmby, P. and Fazio, G. G. and Pahre, M. and Smith, H. A. and Kennicutt, Robert C., Jr. and Calzetti, Daniela and Dale, Daniel A. and Draine, B. T. and Regan, Michael W. and Malhotra, S. and Thornley, Michele D. and Appleton, P. N. and Frayer, D. and Helou, G. and Stolovy, S. and Storrie-Lombardi, L. (2004) Infrared Array Camera (IRAC) Observations of M81. Astrophysical Journal Supplement Series, 154 (1). pp. 222-228. ISSN 0067-0049. https://resolver.caltech.edu/CaltechAUTHORS:20170323-131933186

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Abstract

Infrared Array Camera (IRAC) images of M81 show three distinct morphological constituents: a smooth distribution of evolved stars with bulge, disk, and spiral arm components; a clumpy distribution of dust emission tracing the spiral arms; and a pointlike nuclear source. The bulge stellar colors are consistent with M-type giants, and the disk colors are consistent with a slightly younger population. The dust emission generally follows the blue and ultraviolet emission, but there are large areas that have dust emission without ultraviolet and smaller areas with ultraviolet but little dust emission. The former are presumably caused by extinction, and the latter may be due to cavities in the gas and dust created by supernova explosions. The nucleus appears fainter at 8 μm than expected from ground-based 10 μm observations made 4 years ago.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/422913DOIArticle
http://iopscience.iop.org/article/10.1086/422913PublisherArticle
ORCID:
AuthorORCID
Willner, S. P.0000-0002-9895-5758
Ashby, M. L. N.0000-0002-3993-0745
Barmby, P.0000-0003-2767-0090
Fazio, G. G.0000-0002-0670-0708
Kennicutt, Robert C., Jr.0000-0001-5448-1821
Calzetti, Daniela0000-0002-5189-8004
Dale, Daniel A.0000-0002-5782-9093
Draine, B. T.0000-0002-0846-936X
Malhotra, S.0000-0002-9226-5350
Appleton, P. N.0000-0002-7607-8766
Frayer, D.0000-0003-1924-1122
Helou, G.0000-0003-3367-3415
Storrie-Lombardi, L.0000-0002-5987-5210
Additional Information:© 2004 American Astronomical Society. Received 2004 March 26. Accepted 2004 May 27. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under NASA contract 1407. Support for this work was provided by NASA through contract 1256790 issued by JPL/Caltech. Support for the IRAC instrument was provided by NASA through contract 960541 issued by JPL. M. A. P. acknowledges NASA/LTSA grant NAG5-10777. IRAF is distributed by the National Optical Astronomy Observatories, which are operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Foundation. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASA/JPL/Caltech1407
NASA/JPL/Caltech1256790
JPL960541
NASANAG5-10777
NSFUNSPECIFIED
Subject Keywords:dust, extinction; galaxies: individual (M81) ; galaxies: ISM; galaxies: spiral; galaxies: stellar content; infrared: galaxies
Issue or Number:1
Record Number:CaltechAUTHORS:20170323-131933186
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170323-131933186
Official Citation:S. P. Willner et al 2004 ApJS 154 222
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:75357
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:23 Mar 2017 20:40
Last Modified:09 Mar 2020 13:18

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