A dataset provided by the European Space Agency

Name: A huge ULX bubble in NGC 5585
Published: 2016-07-10T22:00:00Z

Proposal ID	076264
Title	A huge ULX bubble in NGC 5585
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762640101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762640201
DOI	https://doi.org/10.5270/esa-9v8zya2
Principal Investigator, PI	Dr Roberto Soria
Abstract	Accreting black holes release their power through radiation and/or jets. We havediscovered an ultraluminous X-ray source (ULX) in the nearby galaxy NGC 5585,surrounded by a large (diameter virgul300 pc) ionized nebula. We propose a joint XMM-Newton and HST study of this source. With XMM-Newton, we will determine theradiative power of the ULX, its spectral and time variability properties, andconstrain its mass. With HST, we will image the nebula, determine whether it isa jet-inflated ULX bubble, measure its kinetic power and source age, and searchfor an optical counterpart to the black hole.
Publications	A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha, Vineet, Chand, Hum, et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O The ultraluminous X-ray source bubble in NGC 5585 \|Soria, R., Pakull, M. W., et al. \| MNRAS \| 501-1644 \| 2021 \| 2021MNRAS.501.1644S \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.501.1644S 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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2015-06-19T22:50:42Z/2015-06-22T09:39:56Z
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	2016-07-10T22:00:00Z
Keywords	"kinetic power", "optical counterpart", "pc ionized nebula", "XMM", "xmm newton", "huge ulx bubble", "NGC 5585", "time variability properties", "black hole", "ngc 5585", "radiative power", "XMM-Newton", "source age", "HST", "accreting blackhole release"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Roberto Soria, 2016, 'A huge ULX bubble in NGC 5585', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-9v8zya2