From the available observational evidence it appears that X-ray binary sources ... loss and the recoil momentum do change the period and eccentricity of the orbit. ...
CRAB. SS433. Mkn 501. GX339-4. SS433. CRAB. VELA ... Single armed cable. 20.595 m. North branch. 5.220 m. South branch. 5.000 m. BU. SN-1. Shore station ...
... y produce un eclipse, de modo que la fuente de rayos X no se detecta por un breve tiempo. Esos eclipses permiten estimar el per odo orbital del sistema. SS433 ...
Number with really new results 16. Sources of data: EIT (1), MDI (5), VIRGO (4), TSI ... 'SS433' model - what is the out-of-the-ecliptic irradiance? 26a: Floyd ...
Some radio emitting X-ray binary stars in our own galaxy: GRS 1915 105. MERLIN. SS433 ... e.g the pimples on a golf ball at 3000 miles at the highest ...
Title: Conventions Document Issue 3.0 Author: Mitarbeiter Last modified by: Axel M. Quetz Created Date: 1/19/2004 11:18:58 AM Document presentation format
Neutrino astronomy with AMANDA and IceCube Per Olof Hulth Stockholm University hulth@physto.se Content Introduction AMANDA results IceCube expectations Summary Short ...
KVI Seminar, Groningen Neutrino Telescopy in the Mediterranean Sea Towards the km3-Scale Detector KM3NeT Uli Katz Univ. Erlangen 21.02.2005 Introduction
BLACK HOLE. Movie courtesy Wolfgang Steffen, University Guadalajara, Mexico ... The maximum color temperature of the accretion disk is Tcol a (M/ 10M )-1/4 ...
Black holes: observations Lecture 5: Jets and lenses Sergei Popov (SAI MSU) Plan and reviews Jets in AGNs and close binaries Close-by and far-away jets Classification ...
Un sistema binario de rayos X est formado, generalmente, por una estrella ... Izquierda: El microcu sar (dentro del c rculo rojo) y las estrellas del c mulo ...
By Drew Brumm Shocks Strong Shocks Shocks in accretion Compact objects Supernova explosions Accretion of binary systems When does a shock occur When a disturbance ...
INPE Advanced Course on Compact Objects Course IV: Accretion Processes in Neutron Stars & Black Holes Ron Remillard Kavli Center for Astrophysics and Space Research
Contributed papers to ICRC. Response of AMANDA to cosmic ray muons ... derived from known limits on extragalactic protons -ray flux. neutrons can escape ...
R. Svensson Zdziarski AA.Ap.J.349:415-28(1990) ... What is the missing dark matter in the Universe? ... Diameter: 50 cm. Drill 2 holes per week; 16 holes per ...
A inch cube of this material with would weigh more than 100 million tons. ... gradually causes much of the disk material to eventually spiral into the black hole. ...
CRAB. VELA. Galactic. Centre. Need Neutrino Telescopes in both hemispheres to see whole sky ... 16 arms per tower, 20 m arm length, arms 40 m apart. 64 PMs per ...
The sky at radio and visible frequencies: ... Producing a multimedia 'Radio Sky' program ... Development of a STARLAB cylinder presenting the gamma ray sky ...
Supernovae, Gamma-Ray Bursts, and Stellar Rotation S. E. Woosley (UCSC) A. Heger (Univ. Chicago) The Neutrino Powered Wind Duncan, Shapiro, and Wasserman (1986) Qian ...
Results from the Antarctic Muon and Neutrino Detector Array (AMANDA) ... N.B.: Event times scrambled for. blind analysis purposes. 60% of 2000 dataset shown. ...
Gravitation et Trous Noirs Fran oise Combes Observatoire de Paris Gravitation Histoire (suite) Pr dictions et tests Effondrement des toiles Indices de l'existence ...
University of New Mexico, June 13-20, 2006. 4. G. Taylor, Summer Synthesis Imaging ... motion 0.28 mas in 80 days. Tenth Summer Synthesis Imaging Workshop ...
Les campagnes d'observations simultan es. Premiers r sultats sur GRS ... IBIS team, 29 janv. 2003. Campagnes d'observations multi- de MINE. Tr s difficiles ...
Harvard CfA Meeting on GRBs, May 21, 2002. Requirements on the Central Engine ... The Jet-Star. Interaction. Relativistic Jet Propagation Through the Star ...
of 10 s can only traverse 3 x 1011 cm. This is long ... with a (strong classical) gamma-ray burst (though ... Modeled as the 3 x 1052 erg explosion. of a ...
... observation with the VLBA at 20 cm for 40 days (~1/4 of precession period) ... Flag by antenna (most problems are antenna based) Poor weather. Bad playback ...
May 23, 1969 into high earth ... The Vela 5 satellites functioned from July, 1969 to April, 1979 ... bright flash of gamma-rays lasting typically about 20 ...
The Vela 5 satellites functioned from July, 1969 to April, 1979 ... March 3, 1997 (fainter by 20) Groot, Galama, von Paradijs, et al IAUC 6584, March 12, 1997 ...