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

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Standard

Explaining the luminosity spread in young clusters : proto and pre-main sequence stellar evolution in a molecular cloud environment. / Jensen, Sigurd S.; Haugbolle, Troels.

I: Monthly Notices of the Royal Astronomical Society, Bind 474, Nr. 1, 2018, s. 1176-1193.

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Harvard

Jensen, SS & Haugbolle, T 2018, 'Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment', Monthly Notices of the Royal Astronomical Society, bind 474, nr. 1, s. 1176-1193. https://doi.org/10.1093/mnras/stx2844

APA

Jensen, S. S., & Haugbolle, T. (2018). Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment. Monthly Notices of the Royal Astronomical Society, 474(1), 1176-1193. https://doi.org/10.1093/mnras/stx2844

Vancouver

Jensen SS, Haugbolle T. Explaining the luminosity spread in young clusters: proto and pre-main sequence stellar evolution in a molecular cloud environment. Monthly Notices of the Royal Astronomical Society. 2018;474(1):1176-1193. https://doi.org/10.1093/mnras/stx2844

Author

Jensen, Sigurd S. ; Haugbolle, Troels. / Explaining the luminosity spread in young clusters : proto and pre-main sequence stellar evolution in a molecular cloud environment. I: Monthly Notices of the Royal Astronomical Society. 2018 ; Bind 474, Nr. 1. s. 1176-1193.

Bibtex

@article{0e80fe43ea5c4af3ab95999c681faa1e,
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",
year = "2018",
doi = "10.1093/mnras/stx2844",
language = "English",
volume = "474",
pages = "1176--1193",
journal = "Royal Astronomical Society. Monthly Notices",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "1",

}

RIS

TY - JOUR

T1 - Explaining the luminosity spread in young clusters

T2 - proto and pre-main sequence stellar evolution in a molecular cloud environment

AU - Jensen, Sigurd S.

AU - Haugbolle, Troels

PY - 2018

Y1 - 2018

KW - stars: formation

KW - stars: luminosity function

KW - stars: pre-main-sequence

KW - open clusters and associations: individual: Collinder 69, Orion Nebular Cluster

U2 - 10.1093/mnras/stx2844

DO - 10.1093/mnras/stx2844

M3 - Journal article

VL - 474

SP - 1176

EP - 1193

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

SN - 0035-8711

IS - 1

ER -

ID: 191585097