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

dc.contributor.authorHerczeg, Gregory J.
dc.contributor.authorJohnstone, Doug
dc.contributor.authorMairs, Steve
dc.contributor.authorHatchell, Jennifer
dc.contributor.authorLee, Jeong-Eun
dc.contributor.authorBower, Geoffrey C.
dc.contributor.authorChen, Huei-Ru Vivien
dc.contributor.authorAikawa, Yuri
dc.contributor.authorYoo, Hyunju
dc.contributor.authorKang, Sung Ju
dc.contributor.authorKang, Miju
dc.contributor.authorChen, Wen-Ping
dc.contributor.authorWilliams, Jonathan P.
dc.contributor.authorBae, Jaehan
dc.contributor.authorDunham, Michael M.
dc.contributor.authorVorobiov, Eduard I.
dc.contributor.authorZhu, Zhaohuan
dc.contributor.authorRao, Ramprasad
dc.contributor.authorKirk, Helen
dc.contributor.authorTakahashi, Satoko
dc.contributor.authorMorata, Oscar
dc.contributor.authorLacaille, Kevin M.
dc.contributor.authorLane, James
dc.contributor.authorPon, Andy
dc.contributor.authorScholz, Aleks
dc.contributor.authorSamal, Manash R.
dc.contributor.authorBell, Graham S.
dc.contributor.authorGraves, Sarah F.
dc.contributor.authorLee, E'lisa M.
dc.contributor.authorParsons, Harriet
dc.contributor.authorHe, Yuxin
dc.contributor.authorZhou, Jianjun
dc.contributor.authorKim, Mi Ryang
dc.contributor.authorChapman, Scott
dc.contributor.authorDrabek-Maunder, Emily
dc.contributor.authorChung, Eun Jung
dc.contributor.authorEyres, Stewart P.S.
dc.contributor.authorForbrich, Jan
dc.contributor.authorHillenbrand, Lynne A.
dc.contributor.authorInutsuka, Shu Ichiro
dc.contributor.authorKim, Gwanjeong
dc.contributor.authorKim, Kyoung Hee
dc.contributor.authorKuan, Yi-Jehng
dc.contributor.authorKwon, Woojin
dc.contributor.authorLai, Shih Ping
dc.contributor.authorLalchand, Bhavana
dc.contributor.authorLee, Chang Won
dc.contributor.authorLee, Chin-Fei
dc.contributor.authorLong, Feng
dc.contributor.authorLyo, A. Ran
dc.contributor.authorQian, Lei
dc.contributor.authorScicluna, Peter
dc.contributor.authorSoam, Archana
dc.contributor.authorStamatellos, Dimitris
dc.contributor.authorTakakuwa, Shigehisa
dc.contributor.authorTang, Ya-Wen
dc.contributor.authorWang, Hongchi
dc.contributor.authorWang, Yiren
dc.date.accessioned2017-11-14T17:55:59Z
dc.date.available2017-11-14T17:55:59Z
dc.date.issued2017-10-27
dc.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. 1 , 43 . https://doi.org/10.3847/1538-4357/aa8b62
dc.identifier.issn0004-637X
dc.identifier.otherArXiv: http://arxiv.org/abs/1709.02052v1
dc.identifier.otherORCID: /0000-0001-8694-4966/work/62751221
dc.identifier.urihttp://hdl.handle.net/2299/19519
dc.descriptionThis is an author-created, uncopyedited version of an article published in The Astrophysical Journal. The Version of Record is available online at DOI: https://doi.org/10.3847/1538-4357/aa8b62.
dc.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
dc.format.extent7621283
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.subjectastro-ph.SR
dc.subjectastro-ph.GA
dc.subjectastro-ph.IM
dc.titleHow do stars gain their mass? : A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star Forming Regionsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.3847/1538-4357/aa8b62
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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