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Coordinated X-Ray, Ultraviolet, Optical, and Radio Observations of the PSR J1023+0038 System in a Low-mass X-Ray Binary State

Bogdanov, Slavko and Archibald, Anne M. and Bassa, Cees and Deller, Adam T. and Halpern, Jules P. and Heald, George and Hessels, Jason W. T. and Janssen, Gemma H. and Lyne, Andrew G. and Moldόn, Javier and Paragi, Zsolt and Patruno, Alessandro and Perera, Benetge B. P. and Stappers, Ben W. and Tendulkar, Shriharsh P. and D'Angelo, Caroline R. and Wijnands, Rudy (2015) Coordinated X-Ray, Ultraviolet, Optical, and Radio Observations of the PSR J1023+0038 System in a Low-mass X-Ray Binary State. Astrophysical Journal, 806 (2). Art. No. 148. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20150803-090609185

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Abstract

The PSR J1023+0038 binary system hosts a neutron star and a low-mass, main-sequence-like star. It switches on year timescales between states as an eclipsing radio millisecond pulsar and a low-mass X-ray binary (LMXB). We present a multi-wavelength observational campaign of PSR J1023+0038 in its most recent LMXB state. Two long XMM-Newton observations reveal that the system spends ~70% of the time in a ≈3 × 10^(33) erg s^(−1) X-ray luminosity mode, which, as shown in Archibald et al., exhibits coherent X-ray pulsations. This emission is interspersed with frequent lower flux mode intervals with ≈5 x 10^(32) erg s^(−1) and sporadic flares reaching up to ≈10^(34) erg s^(−1), with neither mode showing significant X-ray pulsations. The switches between the three flux modes occur on timescales of order 10 s. In the UV and optical, we observe occasional intense flares coincident with those observed in X-rays. Our radio timing observations reveal no pulsations at the pulsar period during any of the three X-ray modes, presumably due to complete quenching of the radio emission mechanism by the accretion flow. Radio imaging detects highly variable, flat-spectrum continuum radiation from PSR J1023+0038, consistent with an origin in a weak jet-like outflow. Our concurrent X-ray and radio continuum data sets do not exhibit any correlated behavior. The observational evidence we present bears qualitative resemblance to the behavior predicted by some existing "propeller" and "trapped" disk accretion models although none can account for key aspects of the rich phenomenology of this system.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/806/2/148DOIArticle
http://iopscience.iop.org/0004-637X/806/2/148PublisherArticle
http://arxiv.org/abs/1412.5145arXivDiscussion Paper
Additional Information:© 2015 American Astronomical Society. Received 2014 December 16; accepted 2015 April 16; published 2015 June 15. A.M.A. and J.W.T.H. acknowledge support from a Vrije Competitie grant from NWO. A.T.D. acknowledges support from an NWO Veni Fellowship. J.W.T.H. and A.P. acknowledge support from NWO Vidi grants. J.W.T.H. also acknowledges funding from an ERC Starting Grant "DRAGNET" (337062). A portion of the results presented was based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. This work was based in part on observations obtained at the MDM Observatory, operated by Dartmouth College, Columbia University, Ohio State University, Ohio University, and the University of Michigan. This research is based in part on observations made with ESO Telescopes at the Paranal Observatory under programme ID 292-5011. The WSRT is operated by ASTRON (Netherlands Institute for Radio Astronomy) with support from The Netherlands Foundation for Scientific Research. Access to the Lovell Telescope is supported through an STFC consolidated grant. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. The EVN (http://www.evlbi.org) is a joint facility of European, Chinese, South African, and other radio astronomy institutes funded by their national research councils. LOFAR, the Low Frequency Array designed and constructed by ASTRON, has facilities in several countries, that are owned by various parties (each with their own funding sources), and that are collectively operated by the International LOFAR Telescope (ILT) foundation under a joint scientific policy. This research has made use of the NASA Astrophysics Data System (ADS). Facilities: XMM, Swift
Funders:
Funding AgencyGrant Number
Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)UNSPECIFIED
European Research Council (ERC)337062
ESA Member StatesUNSPECIFIED
NASAUNSPECIFIED
Science and Technology Facilities Council (STFC)UNSPECIFIED
Subject Keywords:pulsars: general; pulsars: individual (PSR J1023+0038); stars: neutron; X-rays: binaries
Record Number:CaltechAUTHORS:20150803-090609185
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20150803-090609185
Official Citation:Coordinated X-Ray, Ultraviolet, Optical, and Radio Observations of the PSR J1023+0038 System in a Low-mass X-Ray Binary State Slavko Bogdanov et al. 2015 ApJ 806 148
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:59149
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:05 Aug 2015 23:41
Last Modified:05 Aug 2015 23:41

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