Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment

Sigurd S. Jensen; Troels Haugbolle

doi:10.1093/mnras/stx2844

Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment

Astrofysik og Planetforskning

16 Citationer (Scopus)

Originalsprog	Engelsk
Tidsskrift	Monthly Notices of the Royal Astronomical Society
Vol/bind	474
Udgave nummer	1
Sider (fra-til)	1176-1193
Antal sider	18
ISSN	0035-8711
DOI	https://doi.org/10.1093/mnras/stx2844
Status	Udgivet - feb. 2018

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10.1093/mnras/stx2844

stx2844Forlagets udgivne version, 4,38 MB
stx2844.pdfForlagets udgivne version, 4,45 MB

https://arxiv.org/pdf/1710.00823.pdfLicens: Andet

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title = "Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment",

keywords = "stars: formation, stars: luminosity function, stars: pre-main-sequence, open clusters and associations: individual: Collinder 69, Orion Nebular Cluster",

author = "Jensen, {Sigurd S.} and Troels Haugbolle",

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DO - 10.1093/mnras/stx2844

M3 - Journal article

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JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

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Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment

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