A dataset provided by the European Space Agency

Name: THE NEW comma BRIGHT comma SOFT INTERMEDIATE POLAR 1RXSJ062518.2+733433
Published: 2008-11-19T00:00:00Z

Proposal ID	020716
Title	THE NEW, BRIGHT, SOFT INTERMEDIATE POLAR 1RXSJ062518.2+733433
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0207160101
DOI	https://doi.org/10.5270/esa-oyz5nk1
Principal Investigator, PI	Mr ANDREAS STAUDE
Abstract	We propose to observe the newly discovered intermediate polar (IP)1RXSJ062518.2+733433. This object is one out of only 5 known IPs showing adistinct soft X-ray component. With XMM.s large effective area we will achievedata with a high spectral and time resolution in X-rays, optical and the nearUV. We thus will determine the spin-period of the white dwarf, the shape andpositions of the extended accretion regions on the white dwarf, and theaccretion geometry, including the mechanisms of interaction between the magneticfield and the accreted matter, and the processes of energy-release. Thestructure of the accretion curtain can be analysed by studying thetime-dependent absorption in both, the hard and soft X-ray components - tracers of material in completely different states.
Publications	The changing accretion states of the intermediate polar MU Camelopardalis \|Staude, A., Schwope, A. D., et al. \| A&A \| 486-899 \| 2008 \| 2008A&A...486..899S \| http://ui.adsabs.harvard.edu/#abs/2008A&A...486..899S 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 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 A Study on White Dwarf Masses in Cataclysmic Variables Based on XMM-Newton and Suzaku Observations \|Yu, Zhuo-Li, Xu, Xiao-Jie, \| RAA \| 22-45003 \| 2022 \| 2022RAA....22d5003Y \| http://ui.adsabs.harvard.edu/#abs/2022RAA....22d5003Y 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	2005-03-31T14:29:08Z/2005-04-01T03:16:36Z
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	2008-11-19T00:00:00Z
Keywords	"magnetic field", "XMM", "time resolution", "energy release", "accreted matter", "spin period", "white dwarf", "accretion geometry", "accretion curtain", "accretion region", "time dependent absorption"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr ANDREAS STAUDE, 2008, 'THE NEW comma BRIGHT comma SOFT INTERMEDIATE POLAR 1RXSJ062518.2+733433', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-oyz5nk1