'Ls 5039' presentation slideshows

552 views • 43 slides

P. Charles (SAAO) T. Shahbaz (IAC) C. Zurita (Obs. San Pedro Martir)

OBSERVATIONAL EVIDENCE FOR STELLAR-MASS BLACK HOLES Jorge Casares (IAC). P. Charles (SAAO) T. Shahbaz (IAC) C. Zurita (Obs. San Pedro Martir) R. Hynes (Lousiana State Univ.) D. Steeghs ( Harvard-Smithsonian Center for Astroph.). Impact in Astrophysics.

581 views • 42 slides

Cracow, June 26-30, 2006

Josep M. Paredes. BROAD-BAND EMISSION FROM MICROQUASAR JETS. Cracow, June 26-30, 2006. OUTLINE. How many microquasars we know Non-thermal low energy radiation from MQ jets MQ jets as HE and VHE ? -ray sources: Theoretical point of view

544 views • 40 slides

Microquasars and Unidentified TeV Sources

Microquasars and Unidentified TeV Sources. Chuck Dermer (NRL) Penn State University June, 2008. Microquasars: X-ray binaries with jets. Thanks to Diego Torres for discussions. Refs. and acknowledgments: Felix Mirabel talk; Isabelle Grenier Merida ICRC talk;

495 views • 36 slides

MICROQUASARS

MICROQUASARS. Five international workshops VI in Como, Italy (18-22 Sept. 2006). Felix Mirabel European Southern Observatory. Chile on leave from CEA-Saclay. France. HIGH ENERGY SOURCES IN THE GALACTIC CENTRE. Mirabel, Rodriguez, et al, 1992.

462 views • 30 slides

Gamma-ray Large Area Space Telescope

Gamma-ray Large Area Space Telescope. GLAST Science at Lunch LS 5039 Neutron star or Black hole XRB? Richard Dubois (*) (*) Usual caveats and groveling. Outline. HESS sees LS 5039 in TeV What is/was known about it Reminders about microquasars Evidence for black hole Evidence for pulsar.

368 views • 27 slides

Survey of Micro Quasars

Survey of Micro Quasars. Outline. Reminder: what is a microquasar? Established and Candidate microquasars Gamma ray candidates: LSI +615, LS 5039 As seen in DC2 Models for gamma ray spectra. What and Where. High Mass XRB live near galactic plane Low Mass XRB live in the bulge.

306 views • 21 slides

INTEGRAL Deep Observation of LS I +61 303

INTEGRAL Deep Observation of LS I +61 303. Wim Hermsen 1,2 and Lucien Kuiper 1 1 SRON 2 University of Amsterdam Stanford, First GLAST Science Symposium, 7 february 2007. High-Mass X-ray binary at a distance of 2 kpc

356 views • 20 slides

315 views • 20 slides