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相关论文: Infall and SiO emission in V838 Mon

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We report the discovery of multiple shells around the eruptive variable star V838 Mon. Two dust shells are seen in IRAS and MSX images, which themselves are situated in a shell of CO. This securely establishes V838 Mon as an evolved object.…

天体物理学 · 物理学 2009-11-10 Jacco Th. van Loon , A. Evans , Mark T. Rushton , Barry Smalley

V899 Mon is an eruptive young star showing characteristics of both FUors and EXors. It reached a peak brightness in 2010, then briefly faded in 2011, followed by a second outburst. We conducted multi-filter optical photometric monitoring,…

Archival optical spectra from the Sloan Digital Sky Survey of two optically faint flat spectrum protostars, IRAS 04369+2539 and IRAS 05451+0037, show strong emission-line features including -- notably -- clear and broad emission across…

太阳与恒星天体物理 · 物理学 2015-06-03 Lynne A. Hillenbrand , Gillian R. Knapp , Deborah L. Padgett , Luisa M. Rebull , Peregrine M. McGehee

We report the results of recent multicolor photometry and medium resolution spectroscopy of V838 Mon taken in 2007-2008. In the eclipse-like event in December 2006, the hot B3V type companion disappeared. The event accompanied by…

天体物理学 · 物理学 2008-10-13 Vitaly Goranskij , Alla Zharova , Elena Barsukova , Sergei Fabrika , Azamat Valeev

We report observations of the ro-vibronic transition of SO at 1.707 microns on Io. These data were taken while Io was eclipsed by Jupiter, on four nights between July 2000 and March 2003. We analyze these results in conjunction with a…

天体物理学 · 物理学 2009-11-13 Conor Laver , Imke de Pater , Henry Roe , Darrell Strobel

We report high spatial resolution 11.2 and 18.1 micron imaging of V838 Monocerotis obtained with Gemini Observatory's Michelle instrument in 2007 March. Strong emission is observed from the unresolved stellar core of V838 Mon in our Gemini…

天体物理学 · 物理学 2009-11-13 John P. Wisniewski , Mark Clampin , Karen S. Bjorkman , Richard K. Barry

We have observed the OH 1612-MHz maser emission towards the proto-planetary nebula candidate OH17.7-2.0 that underwent a very strong and unusual outburst in 2003. Phase-referencing data were obtained with the EVN in order to localize the…

天体物理学 · 物理学 2009-04-16 M. Szymczak , A. Bartkiewicz , E. Gerard

Herschel FIR imaging and spectroscopy were taken at several epochs to probe the central point source and the extended environment of V838 Mon. PACS and SPIRE maps were used to obtain photometry of the near and far dust around V838 Mon.…

太阳与恒星天体物理 · 物理学 2016-12-14 K. M. Exter , N. L. J. Cox , B. M. Swinyard , M. Matsuura , A. Mayer , E. De Beck , L. Decin

The unusual variable star V838 Monocerotis underwent an eruption in 2002. It continues to illuminate a spectacular series of light echoes, as the outburst light is scattered from circumstellar dust. V838 Mon has an unresolved B3 V companion…

天体物理学 · 物理学 2008-11-26 Melike Afşar , Howard E. Bond

Archival observations of the progenitor of V838 Mon were re-calibrated as well as multiple images from the 2MASS and the DENIS near infrared surveys. Both - the better calibrated values as well as the variability found in the photographic…

天体物理学 · 物理学 2007-05-23 S. Kimeswenger , S. P. S. Eyres

We present Spitzer observations of the unusual variable V838 Monocerotis. Extended emission is detected around the object at 24, 70 and 160um. The extended infrared emission is strongly correlated spatially with the HST optical light echo…

天体物理学 · 物理学 2009-11-11 D. P. K. Banerjee , K. Y. L. Su , K. A. Misselt , N. M. Ashok

We present a type-I outburst of the high-mass X-ray binary EXO 2030+375, detected during INTEGRAL's Performance and Verification Phase in December 2002 (on-source time about 10e+06 seconds). In addition, six more outbursts have been…

天体物理学 · 物理学 2009-11-11 A. Camero Arranz , C. A. Wilson , P. Connell , S. Martínez Núñez , P. Blay , V. Beckmann , V. Reglero

We present a detailed study of V899 Mon (a new member in the FUors/EXors family of young low-mass stars undergoing outburst), based on our long-term monitoring of the source starting from November 2009 to April 2015. Our optical and…

太阳与恒星天体物理 · 物理学 2015-12-09 J. P. Ninan , D. K. Ojha , T. Baug , B. C. Bhatt , V. Mohan , S. K. Ghosh , A. Men'shchikov , G. C. Anupama , M. Tamura , Th. Henning

In 1994 V4332 Sgr underwent a mysterious eruption. Somehow its fast evolution towards a red giant star was, lacking alternative classifications, connected to the red variable M31 RV, which had its eruption in 1988. The red eruptive variable…

天体物理学 · 物理学 2009-11-11 S. Kimeswenger

I review photo-polarimetric and spectropolarimetric observations of V838 Mon, which revealed that it had an asymmetrical inner circumstellar envelope following its 2nd photometric outburst. Electron scattering, modified by pre- or…

天体物理学 · 物理学 2007-05-23 John P. Wisniewski

The occurrence of new FU Orionis-like objects is fundamental to understand the outburst mechanism in young stars and their role in star formation and disk evolution. Our work is aimed at investigating the properties of the recent outburst…

天体物理学 · 物理学 2009-11-13 D. Fedele , M. E. van den Ancker , M. G. Petr-Gotzens , P. Rafanelli

We model the spectra and spectral energy distribution of V838 Mon which were observed in February, March, and November, 2002. Theoretical spectra are calculated using the classical model atmospheres taking into account absorption of atomic…

天体物理学 · 物理学 2007-05-23 Ya. Pavlenko , B. Kaminsky , Yu. Lyubchik , La. Yakovina

We present new observations of the fundamental ro-vibrational CO spectrum of V1647 Ori, the young star whose recent outburst illuminated McNeil's Nebula. Previous spectra, acquired during outburst in 2004 February and July, had shown the CO…

We report high spatial resolution 11.2 and 18.1 micron imaging of the eruptive variable V838 Monocerotis, obtained with Gemini Observatory's Michelle in 2007 March. The 2007 flux density of the unresolved stellar core is roughly 2 times…

天体物理学 · 物理学 2009-11-13 John P. Wisniewski , Mark Clampin , Karen S. Bjorkman , Richard K. Barry , ;

We present a determination of the effective temperatures, iron abundances, and microturbulent velocities for the pseudophotosphere of V838 Mon on 2002 February 25, and March 2 and 26. Physical parameters of the line forming region were…

天体物理学 · 物理学 2009-11-10 B. M. Kaminsky , Ya. V. Pavlenko