ZHANG Yue HXMT Collaboration

Slides:



Advertisements
Similar presentations
X-ray pulsars in wind-fed accretion systems 王 伟 (NAOC) July 2009, Pulsar Summer School Beijing.
Advertisements

Southampton 1 The Disc-Jet connection in LINERS: (and Seyferts..) AMI and X-ray monitoring of M81* Ian M c Hardy, University of Southampton Guy Pooley,
SPIN
Low Mass X-ray Binaries and Accreting Millisecond Pulsars A. Patruno R. Wijnands R. Wijnands M. van der Klis M. van der Klis P. Casella D. Altamirano D.
X-ray pulsars through the eyes of INTEGRAL A.Lutovinov, S.Tsygankov (IKI) & the discussion with J.Poutanen, M.Revnivtsev and V.Suleimanov Funasdalen 2008.
Galloway, Breaking the AMSP mould: HETE J Breaking the AMSP mould: the increasingly strange case of HETE J Duncan Galloway Monash.
Time-distance Helioseismology Technique Issues T. L. Duvall Jr. (NASA/GSFC)
Shu Zhang (on behalf of the HXMT team) Institute of High Energy Physics, Chinese Academy of Science The current status of HXMT and its calibrations.
Neutron Star (Mostly Pulsar) Masses Ingrid Stairs UBC Vancouver CAWONAPS TRIUMF Dec. 9, 2010.
Long-term monitoring of RRAT J HU HuiDong Urumqi Observatory, NAOC July 27, 2009 Rotating Radio Transients Observation.
RXTE and Observations of GC Transients C. B. Markwardt (NASA/GSFC)
Searching for gravitational radiation from Scorpius X-1: Limits from the second LIGO science run Alberto Vecchio on behalf of the LIGO Scientific Collaboration.
Nature of High mass X-ray binaries in the Magellanic Clouds Andry RAJOELIMANANA 1, 2 ‏ Supervisor : Prof Phil CHARLES 1, 2 Co-supervisor : Prof Brian Warner.
Search for Binary Black Holes in Galactic Nuclei Hiroshi SUDOU (Gifu Univ., Japan) EAVN Workshop, Seoul, 2009 March 19.
Maxime KUBRYK, IAP, Ph.D student advisors: Nikos PRANTZOS, IAP Lia ATHANASSOULA, OAMP LIA-ORIGINS, May 2012.
Jamie Holder VERITAS Collaboration Bartol Research Institute/ University of Delaware LS I +61° 303: The High Energy View "Getting Involved with GLAST"
Relativistic Spin Precession in the Double Pulsar Victoria Kaspi McGill University R. Breton, V. Kaspi, M. Kramer, M. McLaughlin, M. Lyutikov, S. Ransom,
©NASA Binary pulsars observed with MAXI T.Mihara, T. Yamamoto, M. Sugizaki (RIKEN) M. Nakajima (Nihon-u) M. Morii, R. Usui, N. Kawai (Tokyo Tech) and the.
Outburst of LS V detected by MAXI, RXTE, Swift Be X-ray Binary LS V INTRODUCTION - Be X-ray Binary consists of a neutron star and Be star.
No Longer! The Double Pulsar Maura McLaughlin West Virginia University 5 April 2012 Collaborators: Kramer (MPiFR), Stairs (UBC), Perera (WVU), Kim (WVU),
Tobias Jogler Max-Planck Institute for Physics Taup 2007 MAGIC Observations of the HMXB LS I in VHE gamma rays Tobias Jogler on behalf of the MAGIC.
1 X-ray enhancement and long- term evolution of Swift J arXiv: Authors: O. Benli, S. Caliskan, U. Ertan et al. Reporter: Fu, Lei.
Long-term properties of Be/X-ray pulsars in the SMC
Topics in X-ray Astronomy Tübingen, Feb XMM-Newton observation of XTE J M.G.F. Kirsch 1), K. Mukerjee 2), M. G. Breitfellner 1), S.
Timing Features of XTE J in 2003 March outburst Fan Zhang et al. (astro-ph/ ) --Possible Evidence for Accreting Blobs.
1 An Impulsive Heating Model for the Evolution of Coronal Loops Li Feng & Weiqun Gan Purple Mountain Observatory.
Nature of X-ray transients in the Magellanic Clouds : (Be/X-ray pulsars, and Supersoft sources) Andry RAJOELIMANANA 1, 2 ‏ Supervisor : Prof Phil CHARLES.
RXTE has doubled the number of known cyclotron lines sources RXTE has observed multiple line sources in outburst RXTE has provided multiple visits to both.
Applying Numerical Relativity and EOB to Black Hole Binary Observation Sean McWilliams NASA Goddard Space Flight Center University of Maryland Collaborators:
SAX J : Witnessing the Banquet of a Hidden Black Widow? Luciano Burderi (Dipartimento di Fisica, Universita’ di Cagliari) Tiziana Di Salvo (Dipartimento.
The Character of High Energy Emission From The Galactic Binary LS Andy Smith Smithsonian Astrophysical Observatory (for the VERITAS collaboration)
Many facets of Neutron Stars Astrosat and beyond Biswajit Paul Raman Research Institute, Bangalore.
The Radio Evolution of the Galactic Center Magnetar Joseph Gelfand (NYUAD / CCPP) Scott Ransom (NRAO), Chryssa Kouveliotou (GWU), Mallory S.E. Roberts.
Star Gobbles Up Its Friend by Universe today Star Eats Companion by ESA news 6 September 2005 Integral and RXTE observations of accreting millisecond pulsar.
IXO and strong gravity Measuring the black hole spin IXO and strong gravity Measuring the black hole spin GiorgioMatt Giorgio Matt (Dipartimento di Fisica.
Twin bunches at FACET-II Zhen Zhang, Zhirong Huang, Ago Marinelli … FACET-II accelerator physics workshop Oct. 12, 2015.
On the role of relativistic effects in the X-ray variability of AGN Piotr Życki Nicolaus Copernicus Astronomical Center, Warsaw, POLAND Andrzej Niedźwiecki.
Dong Li Purple Mountain Observatory, CAS
Composite profile of the Fe Kα spectral line emitted from a binary system of supermassive black holes Predrag Jovanović1, Vesna Borka Jovanović2 and Duško.
Sergei Trushkin , N. Nizhelskij , P. Tsybulev, G. Zhekanis
John Bray PhD candidate Supervisor Dr. J.J Eldridge
“Studying NH variations in Vela X-1”
Cyclotron Resonance Scattering Features in Binary X-ray Pulsars
Nat. Rev. Urol. doi: /nrurol
Observation of microquasars with the MAGIC telescope
Binary Orbits.
The Nature of the Doppler Lines in the Ultra-compact Binary
Speaker:Yi Xie Lunch Talk
XMM-Newton Observation of the composite SNR G0. 9+0
Evolution of X-ray Binaries and the Formation of Binary Pulsars
Center for Gravitational Wave Physics Penn State University
Long Term Variability Of Vela X-1 with RXTE/ASm
In orbit calibration of Insight-HXMT
“The First Spectroscopically Resolved Sup-pc Orbit of a Supermassive Binary Black Hole” E. Bon et al., accepted(?) to ApJ Sarah Burke Spolaor.
On the formation of the peculiar LMXB IGR J in Terzan 5
崔晓红、田文武、朱辉、张孟飞、吴丹、单素素 国家天文台
Insight-HXMT observations on type-I &type-II X-ray bursts
GRB and GRB Two long high-energy GRBs detected by Fermi
Broad-band Spectroscopy of X-ray Binary Pulsars
An overview on HXMT XRB observations/researches
Insight-HXMT observation on Swift J
GALACTIC ASTRONOMY (II): PULSARS
Evolutionary Link between X-ray Pulsars and Millisecond Radio Pulsars
Are there atoll/Z sources in HMXB
Flexural rigidity measured for the biological fin rays (points), scaled 1000 times, and fitted by models of fin rays (lines; see text for discussion of.
Left: Alternations in cardiac output (black) in one typical patient, every 60 s for three cycles, are followed by oscillations in end-tidal CO2 (blue)
Fermi LAT Observations of Galactic X-ray binaries
HXMT in IHEP progresses since last joint calibration meeting
Magnetars with Insight-HXMT
Pulse Nulling and Subpulse Drifting Properties in Pulsars
Presentation transcript:

ZHANG Yue HXMT Collaboration 2018-4-12 Swift J0243.6+6124 ZHANG Yue HXMT Collaboration 2018-4-12

Insight-HXMT observations Swift J0243.6+6124 Be/X-ray binary 2017-10-07 MJD58033 0ks 2018-02-21 MJD58170 1200ks Outline spin evolution orbital elements pulse profile

Pulsar spin evolution HXMT-HE Doroshenko et al.(2017)

Orbit elements T0=MJD58019.17 T0=MJD58019.2 Porb=27.45 d, asini = 115 ls w=85 deg T0=MJD58019.2 Porb=27.36 d, e=0.092, asini = 140 ls w=-76 deg Doroshenko et al.(2017)

Pulse profile Fitting the double peaks Amplitude Phase center FWHM

Pulse profile Pulse profile varies quickly

Summery Spin evolution Orbital elements Pulse profile fdot vs flux