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Related papers: The type Ib supernova 2010O: an explosion in a Wol…

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We present results from a 90 ks Chandra ACIS-S observation of the X-ray luminous interacting galaxy system Arp 299 (NGC 3690/IC 694). We detect 25 discrete X-ray sources with luminosities above 4.0x10^38 erg s^-1 covering the entire Ultra…

Astrophysics of Galaxies · Physics 2016-06-01 K. Anastasopoulou , A. Zezas , L. Ballo , R. Della Ceca

Recently a Type Ic supernova, SN 1998bw, was discovered coincident with a gamma-ray burst, GRB 980425. The supernova had unusual radio, optical, and spectroscopic properties. We explore here models based upon helium stars in the range 9 -…

Astrophysics · Physics 2009-10-30 S. E. Woosley , Ronald G. Eastman , Brian P. Schmidt

We imaged the X-ray error box of GRB 980703, beginning 22.5 hours after the gamma--ray event, in both the optical R and near-infrared H bands. A fading optical/IR object was detected within the X-ray error box, coincident with the variable…

The X-ray transient XMMU J174716.1-281048 was serendipitously discovered with XMM-Newton in 2003. It lies about 0.9 degrees off the Galactic Centre and its spectrum shows a high absorption (~8 x 10E22 cm^(-2)). Previous X-ray observations…

Astrophysics · Physics 2009-11-13 M. Del Santo , L. Sidoli , S. Mereghetti , A. Bazzano , A. Tarana , P. Ubertini

We report a supernova discovery in Ks-band images from the NAOS CONICA adaptive optics (AO) system on the ESO Very Large Telescope (VLT). The images were obtained as part of a near-infrared search for highly-obscured supernovae in the…

The bright, nearby, recently discovered supernova SN2010jl is a member of the rare class of relatively luminous Type~IIn events. Here we report archival HST observations of its host galaxy UGC5189A taken roughly 10yr prior to explosion, as…

We report on Chandra, RXTE, Swift/BAT and MAXI observations of a ~1 day X-ray flare and subsequent outburst of a transient X-ray source observed in October-November 2011 in the globular cluster Terzan 5. We show that the source is the same…

High Energy Astrophysical Phenomena · Physics 2015-06-05 D. Altamirano , L. Keek , A. Cumming , G. R. Sivakoff , C. O. Heinke , R. Wijnands , N. Degenaar , J. Homan , D. Pooley

We present extensive optical and near-infrared photometric and spectroscopic observations of the stripped-envelope (SE) supernova SN 2010as. Spectroscopic peculiarities, such as initially weak helium features and low expansion velocities…

Recent X-ray and radio observations have identified a transient low-mass X-ray binary (LMXB) located only 0.1 pc in projection from the Galactic center, CXOGC J174540.0-290031. In this paper, we report the detailed analysis of X-ray and…

Arp 302, a luminous infrared source (L_{IR} = 4.2x10^{11} Lsun), consisting of two spiral galaxies (VV340A and VV340B) with nuclear separation of 40'', has the highest CO luminosity known. Observations with the BIMA array at 5'' X 7''…

Astrophysics · Physics 2016-08-30 K. Y. Lo , Yu Gao , Robert A. Gruendl

XTE J1739-302 is a transient X-ray source with unusually short outbursts, lasting on the order of hours. Here we give a summary of X-ray observations we have made of this object in outburst with the Rossi X-ray Timing Explorer (RXTE) and at…

We present a Chandra and HST study of IC 10 X-1, the most luminous X-ray binary in the closest starburst galaxy to the Milky Way. Our new hard X-ray observation of X-1 confirms that it has an average 0.5-10 keV luminosity of 1.5e38 erg/s,…

Astrophysics · Physics 2009-11-10 F. E. Bauer , W. N. Brandt

We present results from a 220-ks observation of the galactic supernova remnant (SNR) W49B using the Advanced CCD Imaging Spectrometer (ACIS) on board the Chanrda X-ray Observatory. We exploit these data to perform detailed…

High Energy Astrophysical Phenomena · Physics 2015-06-12 Laura A. Lopez , Enrico Ramirez-Ruiz , Daniel Castro , Sarah Pearson

We present an analysis of XMM-Newton X-ray data of WR30a (WO+O), a close massive binary that harbours an oxygen-rich Wolf-Rayet star. Its spectrum is characterized by the presence of two well-separated broad peaks, or `bumps', one peaking…

High Energy Astrophysical Phenomena · Physics 2015-07-15 S. A. Zhekov , S. L. Skinner

We report on simultaneous observations of the local starburst system Arp 299 with NuSTAR and Chandra, which provides the first resolved images of this galaxy up to energies of ~ 45 keV. Fitting the 3-40 keV spectrum reveals a column density…

After almost 2.5 years of actively accreting, the neutron star X-ray transient and eclipsing binary MXB 1659-29 returned to quiescence in 2001 September. We report on a Chandra observation of this source taken a little over a month after…

We report the discovery of a bright X-ray transient object, XMMU J174554.4-285456, observed in outburst with XMM-Newton on October 3, 2002,and located at 6.3' from SgrA*, the supermassive black hole at the Galactic center.This object…

Astrophysics · Physics 2009-11-10 D. Porquet , N. Grosso , V. Burwitz , I. L. Andronov , B. Aschenbach , P. Predehl , R. S. Warwick

We report on a 63ks Chandra observation of the X-ray transient Swift J195509.6+261406 discovered as the afterglow of what was first believed to be a long duration Gamma-Ray Burst (GRB 070610). The outburst of this source was characterized…

Astrophysics of Galaxies · Physics 2012-03-23 N. Rea , P. G. Jonker , G. Nelemans , J. A. Pons , M. M. Kasliwal , S. R. Kulkarni , R. Wijnands

We investigate iPTF13bvn, a core-collapse (CC) supernova (SN) in the nearby spiral galaxy NGC 5806. This object was discovered by the intermediate Palomar Transient Factory very soon after the explosion and was classified as a…

High Energy Astrophysical Phenomena · Physics 2014-05-21 C. Fremling , J. Sollerman , F. Taddia , M. Ergon , S. Valenti , I. Arcavi , S. Ben-Ami , Y. Cao , S. B. Cenko , A. V. Filippenko , A. Gal-Yam , D. A. Howell

IGR J18483-0311 is a high-mass X-ray binary recently discovered by INTEGRAL. Its periodic fast X-ray transient activity and its position in the Corbet diagram - although ambiguous - led to the conclusion that the source was a likely…

Astrophysics · Physics 2009-11-13 F. Rahoui , S. Chaty
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