The V1647 Ori (IRAS 05436-0007) Protostar and its environment

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dc.contributor.author McGehee, Peregrine
dc.contributor.author Smith, Allyn
dc.contributor.author Henden, Arne
dc.contributor.author Richmond, Michael
dc.contributor.author Knapp, Gillian
dc.contributor.author Finkbeiner, Douglas
dc.contributor.author Ivezic, Zeljko
dc.contributor.author Brinkmann, Jonathan
dc.date.accessioned 2008-11-19T15:24:56Z
dc.date.available 2008-11-19T15:24:56Z
dc.date.issued 2004-12-01
dc.identifier.citation Astrophysical Journal 616 (2004) 1058-1064 en_US
dc.identifier.uri http://hdl.handle.net/1850/7546
dc.description Also archived in: arXiv:astro-ph/0408308 v1 Aug 17 2004 en_US
dc.description.abstract We present Sloan Digital Sky Survey and United States Naval Observatory observations of the V1647 Ori protostar and surrounding field near NGC 2068. V1647 Ori, the likely driving source for HH 23, brightened significantly in November 2003. Analysis of SDSS imaging acquired in November 1998 and February 2002 during the quiescent state, recent USNO photometry, and published 2MASS and Gemini data shows that the color changes associated with brightening suggest an EXor outburst rather than a simple dust clearing event. en_US
dc.language.iso en_US en_US
dc.publisher Universtiy of Chicago Press: Astrophysical Journal en_US
dc.relation.ispartofseries vol. 616 en_US
dc.relation.ispartofseries no. 2 en_US
dc.relation.ispartofseries pps. 1058-1064 en_US
dc.subject Stars - formation en_US
dc.subject Stars - pre-main-sequence en_US
dc.subject Stars - circumstelar matter en_US
dc.subject Stars - individual (V1647 Ori, IRAS 05436-0007 en_US
dc.title The V1647 Ori (IRAS 05436-0007) Protostar and its environment en_US
dc.type Article en_US

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