CaltechAUTHORS
  A Caltech Library Service

AKARI and BLAST Observations of the Cassiopeia A Supernova Remnant and Surrounding Interstellar Medium

Sibthorpe, B. and Bock, J. J. (2010) AKARI and BLAST Observations of the Cassiopeia A Supernova Remnant and Surrounding Interstellar Medium. Astrophysical Journal, 719 (2). pp. 1553-1564. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20100831-152351185

[img]
Preview
PDF - Published Version
See Usage Policy.

962Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20100831-152351185

Abstract

We use new large area far infrared maps ranging from 65 to 500 μm obtained with the AKARI and the Balloon-borne Large Aperture Submillimeter Telescope missions to characterize the dust emission toward the Cassiopeia A supernova remnant (SNR). Using the AKARI high-resolution data we find a new "tepid" dust grain population at a temperature of ~35 K and with an estimated mass of 0.06 M_☉. This component is confined to the central area of the SNR and may represent newly formed dust in the unshocked supernova ejecta. While the mass of tepid dust that we measure is insufficient by itself to account for the dust observed at high redshift, it does constitute an additional dust population to contribute to those previously reported. We fit our maps at 65, 90, 140, 250, 350, and 500 μm to obtain maps of the column density and temperature of "cold" dust (near 16 K) distributed throughout the region. The large column density of cold dust associated with clouds seen in molecular emission extends continuously from the surrounding interstellar medium to project on the SNR, where the foreground component of the clouds is also detectable through optical, X-ray, and molecular extinction. At the resolution available here, there is no morphological signature to isolate any cold dust associated only with the SNR from this confusing interstellar emission. Our fit also recovers the previously detected "hot" dust in the remnant, with characteristic temperature 100 K.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/719/2/1553DOIUNSPECIFIED
http://iopscience.iop.org/0004-637X/719/2/1553PublisherUNSPECIFIED
Additional Information:© 2010 Received 2009 October 5; accepted 2010 April 20; published 2010 August 2. We acknowledge the support of NASA through grant numbers NAG5-12785, NAG5-13301, and NNGO-6GI11G, the NSF Office of Polar Programs, the Canadian Space Agency, the Natural Sciences and Engineering Research Council (NSERC) of Canada, the UK Science and Technology Facilities Council (STFC), and Korea Science and Engineering Foundation (R01- 2007-000-20336-0, F01-2007-000-10048-0). This work is also based on observations with AKARI, a JAXA project with the participation of ESA. Finally, we acknowledge M. Wright for the use of his 83 GHz radio map of Cas A.
Funders:
Funding AgencyGrant Number
NASANAG5-12785
NASANAG5-13301
NASANNGO-6GI11G
NSFUNSPECIFIED
Canadian Space AgencyUNSPECIFIED
Natural Sciences and Engineering Research Council (NSERC) of CanadaUNSPECIFIED
UK Science and Technology Facilities CouncilUNSPECIFIED
Korea Science and Engineering FoundationR01-2007-000-20336-0
Korea Science and Engineering FoundationF01-2007-000-10048-0
Subject Keywords:early universe; ISM: supernova remnants
Issue or Number:2
Classification Code:PACS: 98.38.Mz; 98.38.Dq; 98.38.Cp; 98.38.Am
Record Number:CaltechAUTHORS:20100831-152351185
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20100831-152351185
Official Citation:B. Sibthorpe et al 2010 ApJ 719 1553 doi: 10.1088/0004-637X/719/2/1553
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:19752
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:03 Sep 2010 18:17
Last Modified:03 Oct 2019 02:01

Repository Staff Only: item control page