A dataset provided by the European Space Agency

Name: Star Formation in the interacting galaxy pair NGC 1512 - NGC 1510
Published: 2013-07-12T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	069316
Title	Star Formation in the interacting galaxy pair NGC 1512 - NGC 1510
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693160101
DOI	https://doi.org/10.5270/esa-8bnswvb
Principal Investigator, PI	Dr Lorenzo Ducci
Abstract	We propose to observe the pair of galaxies NGC 1512/1510 for a total exposuretime of 60 ks. The observation of NGC 1512/1510 will allow us to gaininformation on X-ray Binaries (XRBs) born in the outer arms of NGC 1512, anenvironment with atypical densities and chemical abundances, that is likely toaffect the evolution of XRBs. This observation is also r^ant to theimprovement of our knowledge on the properties of rejuvenated ellipticalgalaxies, such as NGC 1510, in which we expect to observe a population of youngXRBs formed after the recent accretion of material from NGC 1512, superimposedon an older population of Low-Mass X-ray Binaries (LMXBs).
Publications	XMM-Newton observation of the interacting galaxies NGC 1512 and NGC 1510 \|Ducci L. Kavanagh P. J. et al. \| A&A \| 566-115 \| 2014 \| 2014A&A...566A.115D \| http://ui.adsabs.harvard.edu/#abs/2014A&A...566A.115D Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y 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 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 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	EPN, RGS1, OM, RGS2, EMOS1, EMOS2
Temporal Coverage	2012-06-16T20:31:49Z/2012-06-17T16:24:36Z
Version	21.51_20241115_1113
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	2013-07-12T00:00:00Z
Last Update	2026-07-09
Keywords	"ngc 1510", "xrbs formed", "total exposure time", "galaxy ngc 1512", "ngc 1512", "outer arms", "rejuvenated elliptical galaxy", "gain information", "chemical abundance", "NGC 1512", "star formation", "atypical densities"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Lorenzo Ducci, 2013, 'Star Formation in the interacting galaxy pair NGC 1512 - NGC 1510', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-8bnswvb
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.