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

DARK

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

19 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 - 1 jun. 2015

Adgang til dokumentet

10.1093/mnras/stv487

MNRAS-2015-Mattsson-4079-90Forlagets udgivne version, 1,01 MB

Citationsformater

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.; Matsuura, Mikako.

I: Monthly Notices of the Royal Astronomical Society, Bind 449, Nr. 4, 01.06.2015, s. 4079-4090.

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

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AU - Matsuura, Mikako

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