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Proposal ID 008994
Title X-rays from protostars: the next step
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DOI https://doi.org/10.5270/esa-cz9z83r
Principal Investigator, PI Dr Thierry Montmerle
Abstract X-rays have been detected from Class I protostars, which are understood from IR and mm data to be evolved protostars at the end of the accretion phase, when the central star is essentially formed (age ~ 10E5 yrs). We propose to move one step closer to star formation by observing Class 0 protostars, which are at a much earlier stage (age ~10E4 yrs). We select a sample of 5 protostars for which the extinction is known to be moderate (Av ~ 100). Since X-rays probe the innermost regions of protostars, we hope to gain insight for the first time into the nature of the central object, before it becomes a real star.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-03-18T09:16:38Z/2003-10-23T07:29:39Z
Version 21.51_20241115_1113
Mission Description The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 2004-11-11T00:00:00Z
Last Update 2026-07-09
Keywords "x rays", "10e4 yrs", "accretion phase", "moderate av", "10e5 yrs", "innermost region", "evolved protostars", "move step closer", "central star", "`` class", "formed age", "central object", "stage age", "gain insight", "star formation", "mm data", "'' protostars"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Thierry Montmerle, 2004, 'X-rays from protostars: the next step', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-cz9z83r
Rights Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.