papers

Publications (7)

astro-ph2005

The Nature of Nonthermal X-ray Filaments Near the Galactic Center

F. Yusef-Zadeh, M. Wardle, M. Muno +2

Recent Chandra and XMM-{\it Newton} observations reported evidence of two X-ray filaments G359.88-0.08 (SgrA-E) and G359.54+0.18 (the ripple filament) near the Galactic center. The…

astro-ph2007

GRB 070201: A possible Soft Gamma Ray Repeater in M31

E. O. Ofek, M. Muno, R. Quimby +13

The gamma-ray burst (GRB) 070201 was a bright short-duration hard-spectrum GRB detected by the Inter-Planetary Network (IPN). Its error quadrilateral, which has an area of 0.124 sq…

astro-ph2008

Results from an extensive simultaneous broadband campaign on the underluminous active nucleus M81*: further evidence for mass-scaling accretion in black holes

S. Markoff, M. Nowak, A. Young +13

We present the results of a broadband simultaneous campaign on the nearby low-luminosity active galactic nucleus M81*. From February through August 2005, we observed M81* five time…

astro-ph2005

A Hot Helium Plasma in the Galactic Center Region

R. Belmont, M. Tagger, M. Muno +2

Recent X-ray observations by the space mission Chandra confirmed the astonishing evidence for a diffuse, hot, thermal plasma at a temperature of 9. K (8 keV) found by previo…

astro-ph2000

Faint Infrared Flares from the Microquasar GRS 1915+105

S. Eikenberry, K. Matthews, M. Muno +3

We present simultaneous infrared and X-ray observations of the Galactic microquasar GRS 1915+105 using the Palomar 5-m telescope and Rossi X-ray Timing Explorer on July 10, 1998 UT…

astro-ph2006

The Origin of Diffuse X-ray and -ray Emission from the Galactic Center Region: Cosmic Ray Particles

F. Yusef-Zadeh, M. Muno, M. Wardle +1

(Abridged) The inner couple hundred pcs of our Galaxy is characterized by significant amount of synchrotron-emitting gas, which appears to co-exist with a large reservoir of molecu…

astro-ph2003

Modulation of the X-ray Fluxes by the AEI

P. Varnière, M. Muno, M. Tagger +1

The Accretion-Ejection Instability (AEI) has been proposed to explain the low frequency Quasi-Periodic Oscillation (QPO) observed in low-mass X-Ray Binaries. Its frequency, typical…