Atjaunināt sīkdatņu piekrišanu

High-Energy Emission from Pulsars and their Systems: Proceedings of the First Session of the Sant Cugat Forum on Astrophysics 2011 ed. [Hardback]

Edited by , Edited by
  • Formāts: Hardback, 644 pages, height x width: 235x155 mm, weight: 1298 g, XXXVI, 644 p., 1 Hardback
  • Sērija : Astrophysics and Space Science Proceedings
  • Izdošanas datums: 04-Feb-2011
  • Izdevniecība: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 3642172504
  • ISBN-13: 9783642172502
Citas grāmatas par šo tēmu:
  • Hardback
  • Cena: 394,10 €*
  • * ši ir gala cena, t.i., netiek piemērotas nekādas papildus atlaides
  • Standarta cena: 463,65 €
  • Ietaupiet 15%
  • Grāmatu piegādes laiks ir 3-4 nedēļas, ja grāmata ir uz vietas izdevniecības noliktavā. Ja izdevējam nepieciešams publicēt jaunu tirāžu, grāmatas piegāde var aizkavēties.
  • Daudzums:
  • Ielikt grozā
  • Piegādes laiks - 4-6 nedēļas
  • Pievienot vēlmju sarakstam
  • Formāts: Hardback, 644 pages, height x width: 235x155 mm, weight: 1298 g, XXXVI, 644 p., 1 Hardback
  • Sērija : Astrophysics and Space Science Proceedings
  • Izdošanas datums: 04-Feb-2011
  • Izdevniecība: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 3642172504
  • ISBN-13: 9783642172502
Citas grāmatas par šo tēmu:
The aim of the inaugural meeting of the Sant Cugat Forum on Astrophysics was to address, in a global context, the current understanding of and challenges in high-energy emissions from isolated and non-isolated neutron stars, and to confront the theoretical picture with observations of both the Fermi satellite and the currently operating ground-based Cherenkov telescopes. Participants have also discussed the prospects for possible observations with planned instruments across the multi-wavelength spectrum (e.g. SKA, LOFAR, E-VLT, IXO, CTA) and how they will impact our theoretical understanding of these systems. In keeping with the goals of the Forum, this book not only represents the proceedings of the meeting, but also a reflection on the state-of-the-art in the topic.
Radio Pulsar Phenomenology
1(20)
Simon Johnston
Aris Karastergiou
1 Introduction
1(1)
2 Observational Basics
2(2)
3 Integrated profiles and polarization
4(4)
3.1 Pulse width
5(1)
3.2 Profile shape
5(1)
3.3 Linear polarization
6(1)
3.4 Position angle swing and orthogonal modes
7(1)
3.5 Circular polarization
7(1)
4 Rotating Vector Model
8(2)
5 Problems and Perils of the RVM
10(1)
6 Radius-to-Frequency mapping
11(1)
7 Velocity - spin axis alignment
12(1)
8 Beam models
12(2)
8.1 Rankin et al
12(1)
8.2 Lyne & Manchester
13(1)
8.3 Karastergiou & Johnston
14(1)
9 Two Case Studies
14(2)
9.1 The radio loud magnetars
14(1)
9.2 Pulsars with notches
15(1)
10 Summary
16(1)
11 Future instruments and the Square Kilometre Array
17(4)
References
18(3)
Radio pulsar populations
21(16)
Duncan R. Lorimer
1 Selection effects in radio pulsar surveys
21(3)
1.1 Flux-distance relationship
22(1)
1.2 The radio sky background
22(1)
1.3 Propagation effects in the interstellar medium
22(1)
1.4 Finite size of the emission beam
23(1)
1.5 Pulse nulling
24(1)
1.6 Intermittency
24(1)
2 Correcting the biases in the observed sample
24(2)
3 Recent results
26(6)
3.1 Pulsar space distribution
26(2)
3.2 Pulsar velocities
28(1)
3.3 Pulsar luminosities
28(2)
3.4 Magnetic alignment
30(1)
3.5 Magnetic field decay
31(1)
4 Final thoughts and future prospects
32(5)
4.1 Rotating radio transients
32(1)
4.2 Millisecond pulsars
32(1)
4.3 Pulsars in the Magellanic Clouds
33(1)
4.4 Globular cluster pulsars
33(1)
References
34(3)
Pulsar Results with the Fermi Large Area Telescope
37(20)
Paul S. Ray
Pablo M. Saz Parkinson
1 Introduction
37(2)
1.1 Gamma-ray Pulsars in the Year 2000
37(1)
1.2 Fermi and AGILE
38(1)
2 The EGRET Pulsars in Exquisite Detail
39(3)
3 Young Pulsars Found Using Radio Ephemerides
42(1)
4 Millisecond Pulsars
42(4)
4.1 Radio MSPs
43(1)
4.2 Searches of LAT Unassociated Sources
44(1)
4.3 Globular Cluster MSPs
45(1)
5 Blind Periodicity Searches
46(2)
6 Pulsar Timing with the LAT
48(1)
7 Multiwavelength Connections
49(3)
8 The LAT Pulsar Population
52(2)
9 Future Expectations
54(3)
References
55(2)
Fermi view of the EGRET pulsars
57(6)
F. Gargano
1 Introduction
57(1)
2 Analysis results
58(3)
3 Conclusion
61(2)
References
61(2)
"Garden-variety" Gamma-ray Pulsars J0248+6021 & J2240+5832
63(6)
David A. Smith
1 Introduction
63(1)
2 Two Not-So-Typical Pulsars
64(1)
3 About those distances
64(1)
4 Understanding the Beams
65(1)
5 Conclusions
66(3)
References
67(2)
Extension studies of galactic sources with Fermi
69(6)
Francesco Giordano
1 The simulated cases
69(3)
2 Galactic extended SNRs: the W51C, the W44 and the IC443
72(1)
3 Conclusions
73(2)
References
73(2)
Advances in understanding double features in radio pulsar profiles
75(4)
Jaroslaw Dyks
Bronislaw Rudak
Paul Demorest
1 The Double Features
75(1)
2 The interpretation
76(3)
References
78(1)
Emission from the Polar Cap and Slot Gap
79(20)
Alice K. Harding
Isabelle A. Grenier
1 Introduction
79(1)
2 Polar cap and slot gap electrodynamics
80(4)
2.1 Polar cap pair cascades
81(1)
2.2 The slot gap
82(2)
3 Geometry of high-energy radiation
84(1)
4 Confronting the Fermi observations
85(11)
4.1 Spectra
86(1)
4.2 Population synthesis and light curve fitting
87(7)
4.3 New insights from the increasing γ-ray MSP Population
94(2)
5 Learning from Nature - Future pulsar modeling
96(3)
References
97(2)
Gamma-ray emission and pair creation of outer gap
99(18)
K. S. Cheng
1 Introduction
99(1)
2 Two dimensional outergap model
100(8)
2.1 Gap structure
101(2)
2.2 Curvature radiation spectrum
103(1)
2.3 Properties of curvature spectra with gap parameters
104(1)
2.4 Fitting Results
105(3)
3 Pair creation mechanisms
108(7)
3.1 Photon-photon pair-creation process
108(1)
3.2 New gap closure mechanism
109(3)
3.3 Predictions of new outer gap model
112(3)
4 Summary
115(2)
References
115(2)
What Pulsar High-Energy Emission Model Survives?
117(22)
Kouichi Hirotani
1 Introduction
117(3)
2 Basic equations
120(5)
2.1 Poisson Equation for Electrostatic Potential
120(2)
2.2 Particle Boltzmann Equations
122(1)
2.3 Radiative Transfer Equation
123(1)
2.4 Boundary Conditions
124(1)
3 Self-consistent OG solution: the case of the Crab pulsar
125(1)
3.1 Gap geometry and acceleration electric field
125(1)
3.2 Photon mapping result and radiation spectrum
125(1)
4 Slot-gap model: the case of the Crab pulsar
126(7)
4.1 Formation of a slot gap in the polar-cap region
127(2)
4.2 Lower-altitude slot-gap solution
129(1)
4.3 Higher-altitude slot-gap model
130(3)
5 Discussion
133(6)
References
134(5)
Current Models of Pulsar Magnetospheres
139(20)
Anatoly Spitkovsky
1 Introduction
139(1)
2 Plasma supply and charge-separated models
140(2)
3 Force-free models
142(7)
4 Implications of the magnetospheric solutions
149(10)
4.1 Consequences for spin down
149(1)
4.2 High energy emission
150(3)
4.3 Reconnection and time-dependence
153(1)
4.4 Current structure and origin
154(1)
4.5 Differential rotation
155(1)
4.6 Conclusion
156(1)
References
156(3)
Modeling of γ-ray Pulsar Light Curves from Force-Free Magnetosphere
159(6)
Xue-Ning Bai
Anatoly Spitkovsky
References
163(2)
A Tale of Two Current Sheets
165(16)
Jonathan Arons
1 Follow The Energy
165(11)
2 Follow the Mass
176(5)
References
179(2)
The high-energy emission from the pulsar striped wind
181(4)
Jerome Petri
1 Introduction
181(1)
2 The striped wind model
182(1)
3 Application to γ-ray pulsars
183(2)
References
184(1)
Gamma-rays from millisecond pulsars in Globular Clusters
185(22)
Wlodek Bednarek
1 Introduction
185(1)
2 The stellar content of Globular Clusters
186(1)
3 Compact objects within Globular Clusters
187(2)
3.1 Millisecond pulsars
187(1)
3.2 Cataclysmic Variables and LMXBs
188(1)
3.3 Intermediate mass black holes?
188(1)
4 Non-thermal emission from Globular Clusters
189(2)
4.1 Low energy radiation
189(1)
4.2 Gamma-rays
189(2)
5 Models for gamma-ray emission
191(9)
5.1 Interpretation of the observed GeV γ-ray emission
192(1)
5.2 TeV γ-ray emission from MSP winds and shocks
193(4)
5.3 Constraints on the MSP population
197(3)
6 Gamma-rays from electrons injected from other sources?
200(2)
7 Conclusions
202(5)
References
204(3)
Modelling the Growing Population of γ-ray Millisecond Pulsars
207(6)
C. Venter
A. K. Harding
T. J. Johnson
1 Introduction
207(1)
2 Pulsar Models
208(2)
3 Results
210(1)
4 Discussion and Conclusions
210(3)
References
210(3)
A Joint Radio Gamma-ray Variability Study of the Crab Pulsar
213(6)
Glenn Jones
Ryan Shannon
1 Introduction
213(1)
2 Radio Observations
214(1)
2.1 Signal Processing
214(1)
3 Gamma-Ray Radio Correlation
215(4)
References
217(2)
AGILE observations of PSR B1509-58
219(6)
M. Pilia
A. Pellizzoni
1 Introduction
219(1)
2 AGILE Observations, Data Analysis and Results
220(1)
3 Discussion
221(4)
References
223(2)
Understanding the fundamental parameters of millisecond pulsars
225(4)
Benoit Pancrazi
1 Introduction
225(2)
2 Observations and data analysis
227(1)
3 Discussion and conclusion
227(2)
References
228(1)
Pulsars as gravitational wave detectors
229(18)
George Hobbs
1 Introduction
229(1)
2 Using pulsars to search for GWs
230(4)
3 Current data sets
234(2)
4 Potential sources of gravitational waves
236(5)
4.1 Single sources
236(2)
4.2 Burst sources
238(1)
4.3 Stochastic background
239(2)
5 Accessing pulsar data sets
241(1)
6 The future
241(1)
7 Conclusion
242(5)
References
242(5)
Magnetar outbursts: an observational review
247(28)
Nanda Rea
Paolo Esposito
1 Author's preface
247(1)
2 A bit of history
248(2)
3 General observational characteristics
250(1)
4 Multiband view of magnetars
250(4)
4.1 Radio emission of magnetars
251(2)
4.2 Optical and infrared emission of magnetars
253(1)
4.3 Soft X-ray emission of magnetars
253(1)
4.4 Hard X-ray emission of magnetars
254(1)
5 Magnetars' Outbursts
254(10)
5.1 XTEJ1810-197
255(1)
5.2 IE 1547-5408
256(2)
5.3 AXJ1844-0258
258(1)
5.4 1E2259+586
258(1)
5.5 IE 1048.1-5937
259(1)
5.6 CXOUJ1647-4552
260(1)
5.7 4U0142+614
260(1)
5.8 SGR 1806-20
261(1)
5.9 SGR 1627-41
262(1)
5.10 SGR 0501+4516
263(1)
5.11 SGR 0418+5729
263(1)
5.12 SGR 1833-0832
264(1)
6 Conclusions
264(11)
References
265(10)
Wide-band X-ray Studies of Magnetars with Suzaku
275(4)
T. Enoto
K. Makishima
N. Rea
Y. E. Nakagawa
K. Nakazawa
T. Sakamoto
1 Suzaku Observations of Magnetars
275(2)
2 Spectral Evolution of Magnetars
277(2)
References
278(1)
Bursts and Flares from Highly Magnetic Pulsars
279(20)
GianLuca Israel
Simone Dall'Osso
1 MAGnetic NEutron sTARS
280(2)
2 SGRs Giant Flares and their magnetic fields
282(3)
2.1 The Cavallo-Fabian-Rees Variability Limit
284(1)
3 SGRs Intermediate Flares in the Swift era
285(14)
3.1 The March 2006 Burst Storm of SGR 1900+14
287(6)
3.2 Further Observations: the case of SGR 0501+4516 and 1E 1547.0-5408
293(4)
References
297(2)
Activated Magnetospheres of Magnetars
299(24)
Andrei M. Beloborodov
1 Introduction
299(2)
2 Electrodynamics of untwisting
301(5)
2.1 Evolution equation for axisymmetric twist
301(2)
2.2 j-bundle
303(3)
3 Transient magnetars
306(5)
3.1 Magnetospheric activity or deep crustal heating?
306(1)
3.2 Individual objects
307(4)
4 Pair creation
311(2)
5 Plasma circulation in the magnetosphere
313(4)
6 Magnetospheric emission
317(3)
7 Conclusions
320(3)
References
320(3)
Suzaku Detection of Hard X-ray Emission in SGR 0501+4516 Short Burst Spectrum
323(6)
Yujin E. Nakagawa
Teruaki Enoto
Kazuo Makishima
Atsumasa Yoshida
Kazutaka Yamaoka
Takanori Sakamoto
Nanda Rea
Kevin Hurley
1 Introduction
324(1)
2 Hard X-ray Emission in Burst Spectra
324(1)
3 Discussion
325(4)
References
326(3)
The magnetar emission in the IR band: the role of magnetospheric currents
329(8)
Silvia Zane
Luciano Nobili
Roberto Turolla
1 Introduction
329(1)
2 Pair production in the inner magnetosphere
330(2)
3 IR/Optical emission
332(1)
4 Discussion and Conclusion
333(4)
References
334(3)
Double features in mean pulsar profiles and the nature of their radio emission
337(4)
George I. Melikidze
Janusz Gil
1 Frequency dependence of the bifurcation angle
337(2)
2 Energy considerations
339(2)
References
340(1)
Can the magnetic field of long-period X-ray pulsars be supercritical?
341(4)
N.R. Ikhsanov
N.G. Beskrovnaya
1 Magnetar hypothesis
341(2)
2 Feedback hypothesis
343(2)
References
344(1)
X-ray emission from isolated neutron stars
345(20)
Sandro Mereghetti
1 Introduction
345(2)
2 Origin of the X-ray emission in isolated neutron stars
347(1)
3 The X-ray Dim Isolated Neutron Stars
348(3)
4 Central Compact Objects in Supernova Remnants
351(1)
5 The Magnetar candidates: Anomalous X-ray Pulsars and Soft Gamma-ray Repeaters
352(4)
6 Rotating Radio Transients
356(1)
7 Rotation-powered pulsars with high magnetic field
357(1)
8 Conclusions
358(7)
References
359(6)
X-ray thermal radiation from hot polar cap in pulsars
365(4)
Janusz Gil
George I. Melikidze
1 Introduction
365(1)
2 Surface magnetic field
366(1)
3 Drifting subpulses
367(2)
References
368(1)
Radio polarization of RRAT J1819-1458
369(4)
A. Karastergiou
1 Introduction
369(1)
2 Polarization characteristics
370(2)
3 Discussion and conclusions
372(1)
References
372(1)
Multiwavelength Observations of Pulsar Wind Nebulae
373(20)
Patrick Slane
1 Introduction
373(1)
2 Dynamical Evolution of PWNc
374(3)
3 Spectral Evolution of PWNc
377(2)
4 Case Studies
379(11)
4.1 3C 58
379(3)
4.2 Vela X
382(2)
4.3 G327.1-1.1
384(3)
4.4 HESS J1640-465
387(3)
5 Summary
390(3)
References
390(3)
Multi-wavelength Observations of Composite Supernova Remnants
393(6)
Tea Temim
1 Introduction
393(1)
2 G54.1+0.3: Expansion into SN Ejecta
394(1)
3 G327.1-1.1: Interaction with the Reverse Shock
395(1)
4 Conclusions
396(3)
References
396(3)
Fermi-LAT Results on Pulsar Wind Nebulae after 1.5 year of Observations
399(14)
M.-H. Grondin
M. Lemoine-Goumard
1 Introduction
399(1)
2 The Crab Nebula
400(2)
3 The Vela-X PWN
402(2)
4 The PWN in MSH 15-52
404(1)
5 PSR J1907+0602 and its TeV PWN
404(1)
6 The PWN HESS J1640-465
405(2)
7 A plausible pulsar wind nebula candidate powered by PSR J1023-5746
407(1)
8 Conclusion
408(5)
References
410(3)
Pulsar Wind Nebulae: The GeV to TeV Connection
413(18)
O. C. de Jager
1 Introduction
413(1)
2 The Crab Nebula in γ-rays
414(3)
2.1 The acceleration limit for electrons in the Crab Nebula
414(2)
2.2 The inverse Compton spectrum of the Crab Nebula - towards the spectral tail
416(1)
3 Accelerated PWN Spectra: Observations of the Cooling Effect
417(2)
4 A Single Spectral Component for the GeV to TeV Emission from the PWN of PSR B1509-58
419(2)
5 Calorimetric GeV emission from PWN
421(1)
6 Discontinuous GeV and TeV Emission from Two-Component PWN
422(2)
6.1 Two-Component Extended Emission from the Vela X PWN
422(1)
6.2 Radio and X-Ray Torii of Vela X near the Termination Shock: Discontinuous Spectra
422(2)
7 HESS J1640-465: Another Two-Component Candidate?
424(2)
8 Conclusions
426(5)
References
428(3)
Extended hard X-ray emission from Vela X
431(4)
Fabio Mattana
Regis Terrier
Diego Gotz
Gabriele Ponti
Laurent Bouchet
Maurizio Falanga
Matthieu Renaud
Stephane Schanne
1 Introduction
431(1)
2 INTEGRAL identification of extended hard X-ray emission
432(2)
3 Combined IBIS/ISGRI and Suzaku/XIS spectral analysis
434(1)
4 Conclusions
434(1)
References
434(1)
Cherenkov Telescopes Results on Pulsar Wind Nebulae and Pulsars
435(18)
Emma de Ona Wilhelmi
1 Introduction
435(4)
2 IACT Technique
439(1)
3 Observations of pulsars with IACTs
440(1)
4 Observations of PWNe with Cherenkov telescopes
441(10)
4.1 Young/Composite Pulsar Wind Nebula
444(3)
4.2 "Relic" Pulsar Wind Nebula
447(2)
4.3 Other PWNe candidates
449(2)
5 Concluding Remarks
451(2)
References
451(2)
Lepton Acceleration in Pulsar Wind Nebulae
453(20)
Matthew G. Baring
1 Introduction
453(2)
2 Lepton Acceleration at Relativistic Shocks
455(9)
2.1 The Monte Carlo Method
457(1)
2.2 Results for Relativistic Shock Acceleration
458(6)
3 The Quasi-Perpendicular Pulsar Wind Termination Shock
464(2)
4 Connecting to PWN Observations
466(4)
5 Conclusions
470(3)
References
470(3)
MHD models of Pulsar Wind Nebulae
473(18)
Niccolo Bucciantini
1 Introduction
473(2)
2 Jet-Torus structure and Inner flow properties
475(7)
2.1 Time variability
480(1)
2.2 Gamma rays
481(1)
3 Evolution of PWNe
482(4)
4 Conclusion
486(5)
References
488(3)
TeV Gamma Ray Survey on the Direction of fermi-LAT Pulsars with the Tibet Air Shower Array
491(6)
M. Amenomori
X. J. Bi
D. Chen
S. W. Cui
Danzengluobu
L. K. Ding
X. H. Ding
C. Fan
C. F. Feng
Zhaoyang Feng
Z. Y. Feng
X. Y. Gao
Q. X. Geng
Q. B. Gou
H. W. Guo
H. H. He
M. He
K. Hibino
N. Hotta
Haibing Hu
H. B. Hu
J. Huang
Q. Huang
H. Y. Jia
L. Jiang
F. Kajino
K. Kasahara
Y. Katayose
C. Kato
K. Kawata
Labaciren
G. M. Le
A. F. Li
H. C. Li
J. Y. Li
C. Liu
Y.-Q. Lou
H. Lu
X. R. Meng
K. Mizutani
J. Mu
K. Munakata
H. Nanjo
M. Nishizawa
M. Ohnishi
I. Ohta
S. Ozawa
T. Saito
T. Y. Saito
M. Sakata
T. K. Sako
M. Shibata
A. Shiomi
T. Shirai
H. Sugimoto
M. Takita
Y. H. Tan
N. Tateyama
S. Torii
H. Tsuchiya
S. Udo
B. Wang
H. Wang
Y. Wang
Y. G. Wang
H. R. Wu
L. Xue
Y. Yamamoto
C. T. Yan
X. C. Yang
S. Yasue
Z. H. Ye
G. C. Yu
A. F. Yuan
T. Yuda
H. M. Zhang
J. L. Zhang
N. J. Zhang
X. Y. Zhang
Y. Zhang
Yi Zhang
Ying Zhang
Zhaxisangzhu
X. X. Zhou
1 Introduction
493(1)
2 Results & Discussion
493(4)
References
494(3)
Fermi results on γ-ray binaries
497(16)
Adam B. Hill
Richard Dubois
Diego F Torres
1 Introduction
498(1)
2 LS 1 +61 303
498(4)
2.1 The original discovery, and further TeV observations: flux, spectrum, periodicity
498(1)
2.2 TeV and X-ray simultaneous observations
499(1)
2.3 The Fermi results on LSI +61°303
500(2)
3 LS 5039
502(1)
3.1 The original discovery, and further TeV observations: flux, spectrum, periodicity
502(1)
3.2 The Fermi results on LS 5039
503(1)
4 Cygnus X-3
503(4)
4.1 Historical observations at high energies
503(1)
4.2 The Fermi results on Cygnus X-3
504(3)
5 Cygnus X-1
507(2)
5.1 Reports of high energy and very high energy emission
508(1)
6 Conclusion
509(4)
References
510(3)
Cherenkov Telescope results on gamma-ray binaries
513(18)
Juan Cortina
1 Introduction
513(1)
2 Detected in VHE: PSR B1259-63, LS 5039 and LS I+6T303
514(5)
2.1 PSR B1259-63/SS2833
514(1)
2.2 LS 5039
515(2)
2.3 LS I+61°303
517(2)
3 Uncertain VHE binaries: Cyg X-1 and HESS J0632+057
519(3)
3.1 Cyg X-1
519(2)
3.2 HESS J0632+057
521(1)
4 Searches for other VHE binaries
522(4)
4.1 Cyg X-3
523(3)
5 Conclusions
526(5)
References
527(4)
γ-ray binaries as non-accreting pulsar systems
531(20)
Diego F. Torres
1 Prologue
531(1)
2 Why is a non-accreting pulsar system a tenable alternative?
532(6)
3 Caveats in the search for X-ray spectral lines
538(2)
4 Caveats in the search for pulsations
540(2)
5 Notes on the theoretical models based on pulsar systems
542(5)
5.1 A perspective on the GeV cutoffs of LS I +61°303 and LS 5039
543(4)
6 Epilogue
547(4)
References
548(3)
Relativistic motion and beamed radiation in gamma-ray binaries
551(4)
Benoit Cerutti
Guillaume Dubus
Gilles Henri
1 Introduction
551(1)
2 Observational backdrop
552(1)
3 Doppler-boosted emission in LS 5039 and LS I +61 303
552(2)
4 Conclusion
554(1)
References
554(1)
A leptonic One-Zone model of the X-Ray/VHE correlated emission in LS I +61 303
555(4)
V. Zabalza
J.M. Paredes
V. Bosch-Ramon
1 Introduction
555(1)
2 Model description and results
556(1)
3 Discussion
557(2)
References
558(1)
New Optical Results on γ-ray Binaries
559(4)
J. Casares
J.M. Corral-Santana
A. Herrero
J.C. Morales
T. Munoz-Darias
I. Negueruela
J.M. Paredes
I. Ribas
M. Ribo
D. Steeghs
L. van Spaandonk
F. Vilardell
1 Introduction
559(1)
2 Revised Orbital Solution in LS 5039
560(1)
3 Probing Binarity in MWC 148
561(2)
References
562(1)
The International X-ray Observatory and other X-ray missions, expectations for pulsar physics
563(22)
Yukikatsu Terada
Tadayasu Dotani
1 Introduction
563(2)
2 Future X-ray Missions
565(5)
2.1 Overview of X-ray Missions
565(1)
2.2 The Small Satellite Missions in 2010s
566(2)
2.3 The ASTRO-H Mission
568(1)
2.4 The International X-ray Observatory
569(1)
3 Pulsar Sciences with Future X-ray Missions
570(10)
3.1 General relativity under strong gravity
570(2)
3.2 Equation of State in neutron stars
572(1)
3.3 Plasma physics under a strong magnetic field
573(2)
3.4 Emission mechanism from Magnetars
575(2)
3.5 Diversity of Pulsar systems: white dwarf pulsars
577(3)
4 Synergy with other wavelength observatories
580(5)
References
581(4)
X-ray Polarimeters
585(26)
Marco Feroci
Paolo Soffitta
1 Neutron Stars Science with X-ray Polarimetry
585(2)
2 Fundamental Parameters of X-ray Polarimetry
587(1)
3 Classical Techniques and Observational Status
588(7)
3.1 Bragg Polarimeters
588(3)
3.2 Thompson/Compton Polarimeters
591(3)
3.3 Observational results
594(1)
4 A jump in sensitivity: the focal plane photoelectric Polarimeters for soft X-rays
595(5)
4.1 The Gas Pixel Detector (GPD) solution
597(1)
4.2 The Time Projection Chamber (TPC) Polarimeter solution
598(2)
5 Observational Prospects
600(7)
5.1 Gravity and Extreme Magnetism SMEX (GEMS)
600(1)
5.2 New Hard X-ray Mission (NHXM)
601(3)
5.3 International X-ray Observatory (IXO)
604(3)
6 Conclusions
607(4)
References
607(4)
New results on high energy cosmic ray electrons observed with Fermi LAT
611(12)
Alexander Moiseev
1 Introduction
611(1)
2 Detection of electrons by LAT
612(5)
3 Result and Discussion
617(3)
4 Conclusion
620(1)
5 Acknowledgements
620(3)
References
620(3)
Positrons From pulsar winds
623
Pasquale Blasi
Elena Amato
1 Introduction
624(2)
2 A pulsar wind inside a supernova remnant
626(3)
3 A pulsar wind escaping the parent supernova remnant: bow shock nebulae
629(2)
4 The positron flux from pulsars
631(6)
5 Discussion
637
References
640