A dataset provided by the European Space Agency

Name 040284
Title X-ray Emission from FU Orionis Stars in Cygnus
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402840101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402840201

DOI 10.5270/esa-pp5pxvc
Author Dr Stephen Skinner
Description FU Orionis objects (FUors) are young low-mass pre-main sequence (PMS) stars that are undergoing accretion at maximum rates 10e-4 solar masses per year. Classical FUors have all experienced optical outbursts attributed to a sudden increase in the disk accretion rate. Very little is known about the X-ray properties of these unusual stars. We initiated a X-ray survey of FUors with XMM-Newton in AO-3 and the prototype FU Ori has been detected. Its X-ray spectrum is very unusual compared to what is typically observed in PMS stars. We propose here to complete our X-ray survey of FU Ors. These observations will allow us to define the X-ray properties of the class and will serve as a valuable historical reference if any of our targets undergoes a future outburst.
Publication X-ray Emission from the FU Orionis Star V1735 Cygni . Skinner, Stephen L., Sokal, Kimberly R., et all. . ApJ . 696-766 . 2009 . 2009ApJ...696..766S ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey . Pineau, F.-X., Motch, C., et all. . A&A . 527-126 . 2011 . 2011A&A...527A.126P ,
Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3 . Ballo, L., Heras, F. J. H., et all. . A&A . 545-66 . 2012 . 2012A&A...545A..66B ,
The Spitzer Mid-infrared Active Galactic Nucleus Survey. I. Optical and Near-infrared Spectroscopy of Obscured Candidates and Normal Active Galactic Nuclei Selected in the Mid-infrared . Lacy, M., Ridgway, S. E., et all. . ApJS . 208-24 . 20...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-07-22T14:26:46Z/2006-10-22T10:47:03Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2007-11-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-11-23T00:00:00Z, 040284, 17.56_20190403_1200. https://doi.org/10.5270/esa-pp5pxvc