A dataset provided by the European Space Agency

Name 055164
Title Pre-planned ToO of a pre-main sequence star undergoing an optical-IR outburst
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551640201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551640301

DOI 10.5270/esa-7g4cjvs
Author Dr Nicolas Grosso
Description Dramatic optical-IR outbursts from PMS stars, which signal the onset of rapid mass-infall onto such stars through their accretion disks, cannot be predicted. However, our Chandra and XMM monitoring of the outburst of V1647 Ori demonstrates that an high accretion rate can also produce an X-ray outburst, and, indeed, that X-ray monitoring of PMS accretion bursts represents a new observational window on the magnetic interaction between the stellar magnetosphere and the accretion disk. We have been allocated Chandra ToO time to monitor with snapshots, beginning just after discovery, any such outbursts during Cycle 9. We propose an 120 ks-exposure XMM ToO of any X-ray outburst confirmed with Chandra to perform X-ray spectroscopy and to investigate X-ray variability on a timescale of a day.
Publication A few days before the end of the 2008 extreme outburst of EX Lupi: accretion shocks and a smothered stellar corona unveiled by XMM-Newton . Grosso, N., Hamaguchi, K., et all. . A&A . 522-56 . 2010 . 2010A&A...522A..56G ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Consistent dust and gas models for protoplanetary disks. IV. A panchromatic view of protoplanetary disks . Dionatos, O., Woitke, P., et all. . A&A . 625-66 . 2019 . 2019A&A...625A..66D ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-08-10T16:14:33Z/2008-08-11T17:04:10Z
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 2009-10-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-10-29T00:00:00Z, 055164, 17.56_20190403_1200. https://doi.org/10.5270/esa-7g4cjvs