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IGR J06074+2205 is a poorly studied X-ray source with a Be star companion. It has been proposed to belong to the group of Be/X-ray binaries. In Be/X-ray binaries, accretion onto the neutron star occurs via the transfer of material from the…

High Energy Astrophysical Phenomena · Physics 2018-06-06 P. Reig , A. Zezas

We present the results obtained from X-ray and optical analysis of the Be/X-ray binary IGR~J06074+2205, focusing on before, during, and after the X-ray outbursts in October and December 2023. The properties of the neutron star in the binary…

High Energy Astrophysical Phenomena · Physics 2024-10-02 Birendra Chhotaray , Sachindra Naik , Gaurava K. Jaisawal , Goldy Ahuja

Present X-ray missions are regularly discovering new X/gamma-ray sources. The identification of the counterparts of these high-energy sources at other wavelengths is important to determine their nature. In particular, optical observations…

Astrophysics of Galaxies · Physics 2015-05-19 P. Reig , A. Zezas , L. Gkouvelis , cat

The accretion-powered millisecond pulsar IGR J00291+5934 underwent two ~10 d long outbursts during 2008, separated by 30 d in quiescence. Such a short quiescent period between outbursts has never been seen before from a neutron star X-ray…

High Energy Astrophysical Phenomena · Physics 2011-01-21 Jacob M. Hartman , Duncan K. Galloway , Deepto Chakrabarty

This study presents a detailed timing analyses of two cataclysmic variables (CVs), [PK2008] HalphaJ115927 and IGR J14091-610, utilizing the optical data from the Transiting Exoplanet Survey Satellite (TESS). Periods of 7.20$\pm$0.02 h,…

Solar and Stellar Astrophysics · Physics 2025-04-23 Arti Joshi

Context. Some of transition disks show asymmetric structures in thermal sub-millimetre emission and optical scattered light. These structures can be the result of planet(s) or companions embedded in the disk. Aims. We aim to detect and…

Earth and Planetary Astrophysics · Physics 2015-11-18 P. Pinilla , J. de Boer , M. Benisty , A. Juhász , M. de Juan Ovelar , C. Dominik , H. Avenhaus , T. Birnstiel , J. H. Girard , N. Huelamo , A. Isella , J. Milli

We present analyses of an Intermediate Polar, IGR J15094-6649, based on the archival optical data obtained from the Transiting Exoplanet Survey Satellite (TESS) and X-ray data obtained from the Suzaku, NuSTAR, and Neil Gehrels Swift…

High Energy Astrophysical Phenomena · Physics 2023-04-19 Arti Joshi , Nikita Rawat , Axel Schwope , J. C. Pandey , Simone Scaringi , D. K. Sahu , Srinivas M Rao , Mridweeka Singh

The stellar binary system LS I +61303, composed of a compact object in an eccentric orbit around a B0 Ve star, emits from radio up to gamma-ray energies. The orbital modulation of radio spectral index, X-ray, and GeV gamma-ray data suggests…

High Energy Astrophysical Phenomena · Physics 2020-10-20 M. Massi , M. Chernyakova , A. Kraus , D. Malyshev , F. Jaron , S. Kiehlmann , S. A. Dzib , R. Sharma , S. Migliari , A. C. S. Readhead

We demonstrate correlated rapid variability between the optical/UV and X-ray emission for the first time in a soft X-ray transient, GRO J1655-40: HST light curves show similar features to those seen by RXTE, but with mean delay of 10-20s.…

Astrophysics · Physics 2009-10-30 R. I. Hynes , K. O'Brien , Keith Horne , W. Chen , C. A. Haswell

We present new observations of the edge-on debris disk around HD 15115 (F star at 48.2 pc) obtained in the near-IR. We search for observational evidence for a second inner planetesimal ring in the system. We obtained total intensity and…

The study of the observational properties of uncommonly long bursts from low luminosity sources with extended decay times up to several tens of minutes is important when investigating the transition from a hydrogen-rich bursting regime to a…

Using the flux resolved spectroscopy for the first time, we analyse the RXTE/PCA data of the black hole X-ray binaries GRS 1915+105 and IGR J17091-3624, when both sources show large amplitude, quasi-regular oscillations in 2.0-60.0 keV…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Mayukh Pahari , Ranjeev Misra , Arunava Mukherjee , J. S. Yadav , S. K. Pandey

We observed the nearly edge-on debris disk system HD 111520 at $J$, $H$, & $K1$ near infrared (NIR) bands using both the spectral and polarization modes of the Gemini Planet Imager (GPI). With these new observations, we have performed an…

The high-mass X-ray binary RX J0146.9+6121, with optical counterpart LS I+61 235 (V831 Cas), is an intriguing system on the outskirts of the open cluster NGC 663. It contains the slowest X-ray pulsar known with a pulse period of around…

PSR J1023+0038 is an exceptional system for understanding how slowly rotating neutron stars are spun up to millisecond rotational periods through accretion from a companion star. Observed as a radio pulsar from 2007-2013, optical data…

High Energy Astrophysical Phenomena · Physics 2015-06-17 A. Patruno , A. M. Archibald , J. W. T. Hessels , S. Bogdanov , B. W. Stappers , C. G. Bassa , G. H. Janssen , V. M. Kaspi , S. Tendulkar , A. G. Lyne

This paper presents observations of the Be/X-ray binary system A0535+26 revealing the first observed loss of its circumstellar disc, demonstrated by the loss of its JHK infrared excess and optical/IR line emission. However optical/IR…

Astrophysics · Physics 2009-10-31 N. J. Haigh , M. J. Coe , I. A. Steele , J. Fabregat

[Abridged] We present and analyze observations of J033241.88-274853.9 at z=0.6679, using multi-wavelength photometry and imaging with FLAMES/GIRAFFE 3D spectroscopy. J033241.88-274853.9 is found to be a blue, young (~320Myr) stellar disk…

Astrophysics · Physics 2009-11-13 M. Puech , F. Hammer , H. Flores , B. Neichel , Y. Yang

We present spectroscopic observations of the X-ray transient XTE J1118+480 acquired during different epochs following the 2000 March outburst. We find that the emission line profiles show variations in their double-peak structure on time…

We present an analysis of long-term optical monitoring observations and optical spectroscopic observations of the counterpart to CXOU J205847.5+414637 (high mass X-ray binary system). We search for a variability in the light curve of Be…

Astrophysics · Physics 2009-11-13 U. Kiziloglu , N. Kiziloglu , A. Baykal , S. K. Yerli , M. Ozbey
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