From flux to dust mass: Does the grain-temperature distribution matter for estimates of cold dust masses in supernova remnants?

Lars Mattsson; Haley L. Gomez; Anja C. Andersen; Mikako Matsuura

doi:10.1093/mnras/stv487

From flux to dust mass: Does the grain-temperature distribution matter for estimates of cold dust masses in supernova remnants?

Lars Mattsson, Haley L. Gomez, Anja C. Andersen, Mikako Matsuura

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16 Citationer (Scopus)

Originalsprog	Engelsk
Tidsskrift	Monthly Notices of the Royal Astronomical Society
Vol/bind	449
Udgave nummer	4
Sider (fra-til)	4079-4090
ISSN	0035-8711
DOI	https://doi.org/10.1093/mnras/stv487
Status	Udgivet - 21 mar. 2015

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10.1093/mnras/stv487

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From flux to dust mass : Does the grain-temperature distribution matter for estimates of cold dust masses in supernova remnants? / Mattsson, Lars; Gomez, Haley L.; Andersen, Anja C. et al.

I: Monthly Notices of the Royal Astronomical Society, Bind 449, Nr. 4, 21.03.2015, s. 4079-4090.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › peer review

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title = "From flux to dust mass: Does the grain-temperature distribution matter for estimates of cold dust masses in supernova remnants?",

keywords = "Stars: AGB and post-AGB, supernovae: general, supernovae: individual: Crab nebula, dust, extinction",

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AU - Mattsson, Lars

AU - Gomez, Haley L.

AU - Andersen, Anja C.

AU - Matsuura, Mikako

PY - 2015/3/21

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KW - Stars: AGB and post-AGB

KW - supernovae: general

KW - supernovae: individual: Crab nebula

KW - dust, extinction

U2 - 10.1093/mnras/stv487

DO - 10.1093/mnras/stv487

M3 - Journal article

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From flux to dust mass: Does the grain-temperature distribution matter for estimates of cold dust masses in supernova remnants?

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