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How do stars gain their mass? : A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star Forming Regions

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contributor authorHerczeg, Gregory J.
contributor authorJohnstone, Doug
contributor authorMairs, Steve
contributor authorHatchell, Jennifer
contributor authorLee, Jeong-Eun
contributor authorBower, Geoffrey C.
contributor authorChen, Huei-Ru Vivien
contributor authorAikawa, Yuri
contributor authorYoo, Hyunju
contributor authorKang, Sung Ju
contributor authorKang, Miju
contributor authorChen, Wen-Ping
contributor authorWilliams, Jonathan P.
contributor authorBae, Jaehan
contributor authorDunham, Michael M.
contributor authorVorobiov, Eduard I.
contributor authorZhu, Zhaohuan
contributor authorRao, Ramprasad
contributor authorKirk, Helen
contributor authorTakahashi, Satoko
contributor authorMorata, Oscar
contributor authorLacaille, Kevin M.
contributor authorLane, James
contributor authorPon, Andy
contributor authorScholz, Aleks
contributor authorSamal, Manash R.
contributor authorBell, Graham S.
contributor authorGraves, Sarah F.
contributor authorLee, E'lisa M.
contributor authorParsons, Harriet
contributor authorHe, Yuxin
contributor authorZhou, Jianjun
contributor authorKim, Mi Ryang
contributor authorChapman, Scott
contributor authorDrabek-Maunder, Emily
contributor authorChung, Eun Jung
contributor authorEyres, Stewart P.S.
contributor authorForbrich, Jan
contributor authorHillenbrand, Lynne A.
contributor authorInutsuka, Shu Ichiro
contributor authorKim, Gwanjeong
contributor authorKim, Kyoung Hee
contributor authorKuan, Yi-Jehng
contributor authorKwon, Woojin
contributor authorLai, Shih Ping
contributor authorLalchand, Bhavana
contributor authorLee, Chang Won
contributor authorLee, Chin-Fei
contributor authorLong, Feng
contributor authorLyo, A. Ran
contributor authorQian, Lei
contributor authorScicluna, Peter
contributor authorSoam, Archana
contributor authorStamatellos, Dimitris
contributor authorTakakuwa, Shigehisa
contributor authorTang, Ya-Wen
contributor authorWang, Hongchi
contributor authorWang, Yiren
date accessioned2017-11-14T17:55:59Z
date available2017-11-14T17:55:59Z
date issued2017-11-01
identifier citationHerczeg , G J , Johnstone , D , Mairs , S , Hatchell , J , Lee , J-E , Bower , G C , Chen , H-R V , Aikawa , Y , Yoo , H , Kang , S J , Kang , M , Chen , W-P , Williams , J P , Bae , J , Dunham , M M , Vorobiov , E I , Zhu , Z , Rao , R , Kirk , H , Takahashi , S , Morata , O , Lacaille , K M , Lane , J , Pon , A , Scholz , A , Samal , M R , Bell , G S , Graves , S F , Lee , E M , Parsons , H , He , Y , Zhou , J , Kim , M R , Chapman , S , Drabek-Maunder , E , Chung , E J , Eyres , S P S , Forbrich , J , Hillenbrand , L A , Inutsuka , S I , Kim , G , Kim , K H , Kuan , Y-J , Kwon , W , Lai , S P , Lalchand , B , Lee , C W , Lee , C-F , Long , F , Lyo , A R , Qian , L , Scicluna , P , Soam , A , Stamatellos , D , Takakuwa , S , Tang , Y-W , Wang , H & Wang , Y 2017 , ' How do stars gain their mass? : A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star Forming Regions ' The Astrophysical Journal , vol 849 , no. 43 . DOI: 10.3847/1538-4357/aa8b62en
identifier issn0004-637X
identifier otherPURE: 12521783
identifier otherPURE UUID: 739f3599-4c0c-4bfc-86dc-dc1930c3e361
identifier otherArXiv: http://arxiv.org/abs/1709.02052v1
identifier urihttp://hdl.handle.net/2299/19519
descriptionThis is an author-created, uncopyedited version of an article published in The Astrophysical Journal. Under embargo. Embargo end date: 1 November 2018. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at DOI: https://doi.org/10.3847/1538-4357/aa8b62.en
description abstractMost protostars have luminosities that are fainter than expected from steady accretion over the protostellar lifetime. The solution to this problem may lie in episodic mass accretion -- prolonged periods of very low accretion punctuated by short bursts of rapid accretion. However, the timescale and amplitude for variability at the protostellar phase is almost entirely unconstrained. In "A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star Forming Regions", we are monitoring monthly with SCUBA-2 the sub-mm emission in eight fields within nearby (en
language isoeng
relation ispartofThe Astrophysical Journalen
rightsen
subjectastro-ph.SRen
subjectastro-ph.GAen
subjectastro-ph.IMen
titleHow do stars gain their mass? : A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star Forming Regionsen
typeArticleen
contributor institutionSchool of Physics, Astronomy and Mathematicsen
contributor institutionCentre for Astrophysics Researchen
identifier doihttp://dx.doi.org/10.3847/1538-4357/aa8b62
description statusPeer revieweden
date embargoedUntil01-11-20


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