A dataset provided by the European Space Agency

Name: The gravitational potential of X-ray Faint Eliptical Galaxy IC1459
Published: 2003-06-06T00:00:00Z

Proposal ID	013598
Title	The gravitational potential of X-ray Faint Eliptical Galaxy IC1459
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0135980201
DOI	https://doi.org/10.5270/esa-m44fjn7
Principal Investigator, PI	Dr Yasushi Fukazawa
Abstract	We found that the gravitational potential of X-ray bright elliptical galaxiesgenerally consists of two components; a small-scale galaxy component and alargely extended component beyond galaxy scale. On the other hand, X-ray faintelliptical galaxies seem to possess only the galaxy-component. If it is true,elliptical galaxies must be classified into two types by only X-rayobservations, and it becomes important for the study of the evolution ofelliptical galaxies. In order to confirm this, we propose to observe an X-rayfaint elliptical galaxy IC1459 with Newton.
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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	2002-04-30T16:45:11Z/2002-05-01T01:53:34Z
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	2003-06-06T00:00:00Z
Keywords	"gravitational potential", "galaxy component", "scale galaxy component", "galaxy scale", "elliptical galaxy"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Yasushi Fukazawa, 2003, 'The gravitational potential of X-ray Faint Eliptical Galaxy IC1459', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-m44fjn7