The V1647 Ori (IRAS 05436-0007) Protostar and its Environment
arXiv:astro-ph/0408308 · doi:10.1086/425069
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.
arXiv comment21 pages, 6 figures, Figure 1 available as color JPEG, accepted by the Astrophysical Journal
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Cited by in corpus (20)
- On the nature of the EXor accretion events: an unfrequent manifestation of a common phenomenology ?
- The Outburst of V1647 Ori Revealed by Spitzer
- V1647 Orionis: Reinvigorated Accretion and the Re-Appearance of McNeil's Nebula
- V1647 Orionis: One Year into Quiescence
- Optical and infrared properties of V1647 Orionis during the 2003-2006 outburst. II. Temporal evolution of the eruptive source
- V1647 Ori: The X-ray Evolution of a Pre-main Sequence Accretion Burst
- A multi-wavelength study of the young star V1118 Orionis in outburst
- Gaia 19ajj: A Young Star Brightening Due to Enhanced Accretion + Reduced Extinction
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- V899 Mon: An Outbursting Protostar With Peculiar Light Curve And Its Transition Phases
- Enhanced X-ray variability from V1647 Ori, the young star in outburst illuminating McNeil's Nebula
- The Continuing Outburst of V1647~Orionis: Winter/Spring 2011 Observations
- Dynamics during outburst: VLTI observations of the young eruptive star V1647 Ori during its 2003-2006 outburst
- Post-Outburst Phase of McNeil's Nebula (V1647 Orionis)
- Optical TiO and VO band emission in two embedded protostars: IRAS 04369+2539 and IRAS 05451+0037
- Gaia 20eae: A newly discovered episodically accreting young star
- X-ray Production by V1647 Ori During Optical Outbursts
- V1647 Orionis (IRAS 05436-0007) : A New Look at McNeil's Nebula
- Post-outburst radio observation of the region around McNeil's nebula (V1647 Ori)
- Near-Infrared Monitoring and Modelling of V1647 Ori in its On-going 2008-12 Outburst Phase