'Radio pulsars' presentation slideshows

The Zoo Of Neutron Stars

The Zoo Of Neutron Stars. Sergei Popov ( SAI MSU ). ( www.bradcovington.com). Neutron stars. Superdense matter, strong gravity and superstrong magnetic fields. Magnetospheric activity. Cooling. Accretion. The old zoo of neutron stars. In 60s the first X-ray sources have been discovered.

607 views • 60 slides

Search for Very High Energy Gamma Ray Emission from Pulsars with H.E.S.S.

Search for Very High Energy Gamma Ray Emission from Pulsars with H.E.S.S. presented by Till Eifert Humboldt University Berlin. Research Seminar WS 2005/06, Experimental High Energy Physics. Outline. Pulsars H.E.S.S. Experiment Timing Analysis Results. Outline. Pulsars

726 views • 53 slides

Papers to read for exams etc.

Papers to read for exams etc. 1 . physics/0503245 Baym, Lamb "Neutron stars" 2 . astro-ph/0405262 Lattimer, Prakash "Physics of neutron stars" 3 . 0705.2708 Weber et al. "Neutron stars interiors and equation of state of superdense matter"

582 views • 47 slides

Radio Astronomy

550 views • 39 slides

NEWS OF PULSAR ASTRONOMY

I.F.MALOV PUSHCHINO RADIOASTRONOMICAL OBSERVATORY, P.N.LEBEDEV PHYSICAL INSTITUTE, RUSSIAN ACADEMY OF SCIENCES. NEWS OF PULSAR ASTRONOMY. PULSARS. Pulsars are sources showing pulsed radiation with regular interval between successive pulses. 1)radio pulsars, 2)X-ray pulsars,

406 views • 39 slides

Lecture 1 Isolated Neutron Stars. Intro.

517 views • 38 slides

One antenna on each side of spacecraft, to see whole sky, i.e., as many GPS satellites at

(Two of these on spacecraft.). Serial communications. One of the two redundant antennae. Power. One antenna on each side of spacecraft, to see whole sky, i.e., as many GPS satellites at a time as possible. Receiver handles them both together. Absolute timestamp end-to-end test.

462 views • 35 slides

Lecture 2 Spin evolution of NSs

485 views • 34 slides

Neutron Star Zoo: radio pulsars, magnetars , RRATs, CCOs, and more

Neutron Star Zoo: radio pulsars, magnetars , RRATs, CCOs, and more. Stephen C.-Y. Ng McGill University. Special thanks to Vicky Kaspi for some materials in this talk. Overview. Since the first pulsar discovered 40 yrs ago, they are all thought to be: b orn spinning fast in SNRs

323 views • 32 slides

Gravitational Wave Detection Using Pulsar Timing Current Status and Future Progress

Gravitational Wave Detection Using Pulsar Timing Current Status and Future Progress. Fredrick A. Jenet Center for Gravitational Wave Astronomy University of Texas at Brownsville. Dick Manchester ATNF/CSIRO Australia. George Hobbs ATNF/CSIRO Australia. KJ Lee Peking U. China.

706 views • 31 slides

Gravitational Wave Detection Using Pulsar Timing Current Status and Future Progress

Gravitational Wave Detection Using Pulsar Timing Current Status and Future Progress. Fredrick A. Jenet Center for Gravitational Wave Astronomy University of Texas at Brownsville. Dick Manchester ATNF/CSIRO Australia. George Hobbs ATNF/CSIRO Australia. KJ Lee Peking U. China.

436 views • 31 slides

Neutron Stars 2: Phenomenology

350 views • 26 slides

Deep X-ray Observations of PSR J1119-6127: Do High- B Pulsars Born with Massive Progenitors?

Deep X-ray Observations of PSR J1119-6127: Do High- B Pulsars Born with Massive Progenitors?. Stephen C.-Y. Ng (HKU) Collaborators: V. M. Kaspi (McGill), W. G. G. Ho (Southampton), P. Weltevrede ( Jodrell Bank), S. Bogdanov (Columbia), R. Shannon (ATNF), & M. E. Gonzalez (UBC).

298 views • 17 slides

Progenitors of Magnetars and Hyperaccreting Magnetized Disks and Central Engines of GRBs

Progenitors of Magnetars and Hyperaccreting Magnetized Disks and Central Engines of GRBs. ???? ? ? ??? ??? ??????????. Gamma-ray bursts: the most violent explosions in the universe! ?. SGR 1806-20. The Formation of a Magnetar.

310 views • 16 slides

Search for Young, Gamma-quiet Pulsars

92 views • 1 slides