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 ~300 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 Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
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
Last Update	2025-08-04
Keywords	"XMM", "source age", "XMM-Newton", "NGC 5585", "accreting blackhole release", "huge ulx bubble", "optical counterpart", "xmm newton", "pc ionized nebula", "kinetic power", "ngc 5585", "black hole", "time variability properties", "HST", "radiative power"
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