'Fe line' presentation slideshows

Review

Review. Exam Review (Questions Beyond Test 1). Question 1. True or False? An increase in income causes the IS curve to shift to the right. Answer 1. False When income changes we move along the IS curve.

634 views • 58 slides

AGN and Surveys with the new X-ray observatories

710 views • 57 slides

Broad iron lines from accretion disks

Broad iron lines from accretion disks. K. Iwasawa University of Cambridge. Accreting black hole systems Most energy dissipates at inner radii of the accretion disk. In the accretion disk + corona model. An X-ray source illuminates the disk to give rise reflection

584 views • 48 slides

Ron Remillard Kavli Center for Astrophysics and Space Research

INPE Advanced Course on Compact Objects Course IV: Accretion Processes in Neutron Stars & Black Holes. Ron Remillard Kavli Center for Astrophysics and Space Research Massachusetts Institute of Technology http://xte.mit.edu/~rr/inpe_IV.2.ppt. IV.2 X-ray States of Black Hole Binaries.

495 views • 37 slides

Accretion and reflection in Galactic BHs and AGNs

Accretion and reflection in Galactic BHs and AGNs. Giovanni Miniutti Lab. Astroparticule et Cosmologie - Paris. The X-ray Universe 2008 - Granada. Accreting black holes: the X-ray view. Soft excess Power law X-ray reflection. e.g. Fabian & Miniutti 07 (CUP review).

365 views • 36 slides

(Some) astrophysical drivers for a high-resolution imaging X-ray spectrometer

350 views • 26 slides

The Non-Flare Temperature and Emission Measure Observed by RHESSI and SXI

The Non-Flare Temperature and Emission Measure Observed by RHESSI and SXI. J.McTiernan (SSL/UCB) J.Klimchuk (NRL) Fall 2003 AGU Meeting. Abstract:

327 views • 21 slides

Line Features in RHESSI Spectra

318 views • 21 slides

A. Streblyanska, G. Hasinger, Finoguenov, X. Barcons, S. Mateos, A. C. Fabian

A relativistic Fe line in the mean X-ray spectra of type-1 and type-2. A. Streblyanska, G. Hasinger, Finoguenov, X. Barcons, S. Mateos, A. C. Fabian.

283 views • 19 slides

NRCO #71: preliminary analysis of MOS data

Mallorca, 8 April 2008 EPIC Calibration Meeting. NRCO #71: preliminary analysis of MOS data. Andrea Tiengo INAF, IASF-Milano. NRCO #71. 3 observations of Tycho SNR: 2007-12-30: medium MOS1: 17 ks MOS2: 19 ks 2008-01-01: CALmedium MOS1: 46 ks MOS2: 36 ks 2008-01-03: CALclosed

178 views • 9 slides

Conclusions

Chi-square (d.o .f.). A systematic analysis of broad Fe lines in bright NS LMXBs with XMM-Newton. M. Cadolle Bel 1 , C. Ng 1, 2 , M. Diaz Trigo 3 and S. Migliari 2. 1 INTEGRAL Science Operation Centre, ESAC, Madrid, SPAIN 2 ESAC, Madrid, SPAIN

132 views • 1 slides