A dataset provided by the European Space Agency

Name: Meet the parents: tracing star formation around the ρ Ophiuchi star.
Published: 2014-09-12T00:00:00Z

Proposal ID	072069
Title	Meet the parents: tracing star formation around the ρ Ophiuchi star.
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720690101
DOI	https://doi.org/10.5270/esa-jsd6e4z
Principal Investigator, PI	Dr Ignazio Pillitteri
Abstract	Understanding the mechanisms that trigger the star formation is of crucialimportance both in the solar neighborhood and in more distant places. We proposean XMM-Newton observation to study a possible case of triggered star formationevent in the nearby star forming region hosting the Rho Ophiuchi star. Thesuburbs of Rho Oph star are depleted of dust and are marked by a warm dust ring.Inside the ring, few young stellar objects with disks are found. Through X-rays,we aim to have a complete census of the disk-less stars more evolved than thosein the main cloud core. Once knowing the sample of stars with and without diskwe can estimate the age and assess the evolutionary stage of this part of thecloud and then trace its star formation history.
Publications	Smooth X-ray variability from rho Ophiuchi A+B. A strongly magnetized primary B2 star? \|Pillitteri Ignazio Wolk Scott J. et al. \| A&A \| 567-4 \| 2014 \| 2014A&A...567L...4P \| http://ui.adsabs.harvard.edu/#abs/2014A&A...567L...4P First stars of the rho Ophiuchi dark cloud. XMM-Newton view of rho Oph and its neighbors \|Pillitteri I. Wolk S. J. et al. \| A&A \| 592-88 \| 2016 \| 2016A&A...592A..88P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...592A..88P The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Evidence for radio and X-ray auroral emissions from the magnetic B-type star u03c1 Oph A \|Leto P. Trigilio C. et al. \| MNRAS \| 493-4657 \| 2020 \| 2020MNRAS.493.4657L \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4657L T Tauri stars as gamma-ray source in the Rho Ophiuchi region \|Filu00f3como A. Escobar G. J. et al. \| BAAA \| 61-213 \| 2020 \| 2020BAAA...61B.213F \| http://ui.adsabs.harvard.edu/#abs/2020BAAA...61B.213F Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-08-29T19:52:04Z/2013-08-30T10:35:24Z
Version	17.56_20190403_1200
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	2014-09-12T00:00:00Z
Last Update	2025-01-27
Keywords	"ophiuchi star ..", "solar neighborhood", "rho oph star", "evolutionary stage", "star formation", "xmm newton", "rho ophiuchi star", "tracing star formation", "complete census", "XMM-Newton", "stellar objects", "main cloud core", "warm dust ring", "star formation history", "XMM", "&# 961"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ignazio Pillitteri, 2014, 'Meet the parents: tracing star formation around the ρ Ophiuchi star.', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jsd6e4z