Supernova Remnants in the Magellanic Clouds. VII. Infrared Emission from Supernova Remnants Export

@article{citeulike:4524842, abstract = {We have used the instruments on the Spitzer Space Telescope to study the Large Magellanic Cloud supernova remnants (SNRs) N11L, N44, N49, N206, N63A, and N157B. The two large SNRs N44 and N206 were not detected in any Spitzer IRAC or MIPS wave bands; the remainder were detected at one or more wavelengths. In particular, the SNRs N49 and N63A each had features that were evident in all available IRAC and MIPS bands. Each of these two also displayed faint limb emission in the MIPS 24 mum band only. Spitzer IRS spectra obtained for the N49 SNR showed a number of prominent lines, with little continuum contribution. We therefore suggest that N49, and possibly N63A, are dominated by line emission, with thermal emission from hot dust being at most a secondary component.}, archivePrefix = {arXiv}, author = {{williams}, R. M. and {chu}, Y. H. and {gruendl}, R.}, citeulike-article-id = {4524842}, citeulike-linkout-0 = {http://arxiv.org/abs/astro-ph/0607598}, citeulike-linkout-1 = {http://arxiv.org/pdf/astro-ph/0607598}, citeulike-linkout-2 = {http://dx.doi.org/10.1086/507839}, citeulike-linkout-3 = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006AJ....132.1877W}, doi = {10.1086/507839}, eprint = {astro-ph/0607598}, journal = {Astron. J.}, keywords = {ir, lmc, mcels, mir, snr, spitzer}, month = {November}, pages = {1877--1889}, posted-at = {2009-05-15 22:03:41}, priority = {5}, title = {{Supernova Remnants in the Magellanic Clouds. VII. Infrared Emission from Supernova Remnants}}, url = {http://dx.doi.org/10.1086/507839}, volume = {132}, year = {2006} }

TY - JOUR ID - citeulike:4524842 L3 - citeulike-article-id:4524842 N2 - We have used the instruments on the Spitzer Space Telescope to study the Large Magellanic Cloud supernova remnants (SNRs) N11L, N44, N49, N206, N63A, and N157B. The two large SNRs N44 and N206 were not detected in any Spitzer IRAC or MIPS wave bands; the remainder were detected at one or more wavelengths. In particular, the SNRs N49 and N63A each had features that were evident in all available IRAC and MIPS bands. Each of these two also displayed faint limb emission in the MIPS 24 mum band only. Spitzer IRS spectra obtained for the N49 SNR showed a number of prominent lines, with little continuum contribution. We therefore suggest that N49, and possibly N63A, are dominated by line emission, with thermal emission from hot dust being at most a secondary component. JF - Astron. J. EP - 1889 TI - {Supernova Remnants in the Magellanic Clouds. VII. Infrared Emission from Supernova Remnants} VL - 132 SP - 1877 KW - ir KW - lmc KW - mcels KW - mir KW - snr KW - spitzer AU - {williams}, RM AU - {chu}, YH AU - {gruendl}, R PY - 2006/November// UR - http://dx.doi.org/10.1086/507839 ER -