A dataset provided by the European Space Agency

Name GT1_kexter_1
Title V838 Mon: aftermath of a stellar merger
URL

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DOI https://doi.org/10.5270/esa-p6hm0rl
Author exter, k.
Description V838 Mon is one of the most enigmatic objects observed in stellarastrophysics in recent decades. It came to attention when it underwenta powerful eruptive outburst in Jan. 2002, increasing in luminosity by afactor of 100 over a period of 3 months. Immediately following this eventa spectacular light echo was formed from the outburst light reflecting offthe surrounding dust. Hubble Space Telescope images following thisexpanding light echo have brought V838 Mon to public attention. Whatmakes V838 Mon an unusual star is that the outburst is not of any typeheretofore seen; the scenarios of a nova-like event or thermonuclearrunaway have been discounted, on the basis of the stellar type andoutburst details. The theories that best explain the outburst are a giantstar engulfing a planetary system or, more likely, a merger between avery low mass star and a very young, maybe pre-main sequencelow-intermediate mass star.Observations show that the envelope of the star expanded in responseto the stellar impact, and than it may now be beginning to contract. ManyO-bearing molecules, dust, an SiO maser and possibly a jet have beenobserved from the star. If the outburst was indeed caused by the mergingof two stars, this is an extremely rare event. Herschel observations ofthis star will allow us to model the kinematics, chemistry, temperatureand density structure of the stellar photosphere and the cool envelopesurrounding the star. These will help answer questions still remainingabout the stellar impact, and will also allow us to understand more abouthow a star responds to such a violent event.
Publication
Instrument SPIRE_SpireSpectrometer_, HIFI_HifiPoint_dbs, SPIRE_SpirePhoto_small, PACS_PacsLineSpec_point, PACS_PacsPhoto_largeScan
Temporal Coverage 2010-09-18T17:33:51Z/2011-10-09T14:34:22Z
Version SPG v14.2.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth cornerstone mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/h®erschel/
Date Published 2012-04-15T00:00:00Z
Last Update 2026-03-02
Keywords Herschel Space Observatory data, ESA Herschel mission dataset, far-infrared astronomy observations, submillimeter astronomy data, infrared space telescope observations, PACS photometer data, PACS spectrometer data, SPIRE photometer data, SPIRE Fourier transform spectrometer data, HIFI heterodyne spectroscopy data, far-infrared spectroscopy dataset, submillimeter spectral line observations, cold universe observations dataset, star formation infrared data, molecular cloud far-infrared observations, interstellar medium spectroscopy data, protoplanetary disk infrared observations, galaxy evolution far-infrared data, dust emission submillimeter observations, cosmic infrared background measurements, extragalactic infrared survey data, calibrated level 2 data products, FITS files astronomy, spectral cubes far-infrared, flux-calibrated maps, continuum photometry data, spectral energy distribution measurements, ESA Herschel Science Archive data
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, exter et al., 2012, 'V838 Mon: aftermath of a stellar merger', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-p6hm0rl