A dataset provided by the European Space Agency

Name: INTRA-BINARY SHOCK &amp; ENERGETICS OF TRANSITIONAL BINARY CANDIDATE PSR J2339-0533
Published: 2018-01-10T23:00:00Z

Proposal ID	079080
Title	INTRA-BINARY SHOCK & ENERGETICS OF TRANSITIONAL BINARY CANDIDATE PSR J2339-0533
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790800101
DOI	https://doi.org/10.5270/esa-1h3zvg8
Principal Investigator, PI	Dr SHRIHARSH P. TENDULKAR
Abstract	In the past two years, three pulsar binaries have shown surprisingback-and-forth transitions between an accreting low mass X-ray binary (LMXB)state and a non-accreting radio millisecond pulsar (MSP) state. These transitional MSPs (tMSPs)overturned the idea that accretion in an LMXB switches off permanently in asingle occurence during pulsar .recycling., but it is unclear how/why thetransitions happen. PSR J2339-0533 is a likely tMSP with spin and orbitparameters very similar to the known tMSPs and shows signs of intermittentaccretion, orbital period and lightcurve variations. These signs suggest thatPSR J2339-0533 may imminently transition into an LMXB. With 150ks NuSTAR and 100ks XMM observations, we propose to establish the pre-transition properties, critical for future work.
Publications	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 ESASky SSOSS: Solar System Object Search Service and the case of Psyche \|Racero, E., Giordano, F., et al. \| A&A \| 659-38 \| 2022 \| 2022A&A...659A..38R \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..38R A Gaia view of the optical and X-ray luminosities of compact binary millisecond pulsars \|Koljonen, Karri I. I., Linares, Manuel, \| MNRAS \| 525-3963 \| 2023 \| 2023MNRAS.525.3963K \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.525.3963K Modeling X-Ray and Gamma-Ray Emission from Redback Pulsar Binaries \|Sim, Minju, An, Hongjun, \| ApJ \| 964-109 \| 2024 \| 2024ApJ...964..109S \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...964..109S 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	2016-12-23T08:27:44Z/2016-12-24T17:14:24Z
Version	19.17_20220121_1250
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	2018-01-10T23:00:00Z
Keywords	"", "NuSTAR", "psr j2339 0533", "XMM", "lmxb switches", "pre transition properties", "intermittent accretion", "orbit parameters", "forth transitions", "imminently transition", "lightcurve variations", "single occurence", "pulsar binary", "intra binary shock", "orbital period", "recycling '"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr SHRIHARSH P. TENDULKAR, 2018, 'INTRA-BINARY SHOCK & ENERGETICS OF TRANSITIONAL BINARY CANDIDATE PSR J2339-0533', 19.17_20220121_1250, European Space Agency, https://doi.org/10.5270/esa-1h3zvg8