Results 101 to 110 of about 167,860 (299)
Binary and Millisecond Pulsars [PDF]
Living Reviews in Relativity, 1998 77 pages, 30 figures, available on-line at http://www.livingreviews.org/lrr-2005 ...
openaire +13 more sources
Interventional therapies for chronic heart failure: An overview of recent developments
ESC Heart Failure, Volume 12, Issue 2, Page 1081-1094, April 2025.Abstract Heart failure (HF), the final manifestation of most cardiovascular diseases, has become a major global health concern, affecting millions of individuals. Despite basic drug treatments, patients present with high morbidity and mortality rates. However, recent advancements in interventional therapy have shown promising results in improving the ...
Bingchen Guo +7 more
wiley +1 more source
Hydrodynamic Interaction between the Be Star and the Pulsar in the TeV Binary PSR B1259-63/LS 2883
, 2011 We study the interaction between the Be star and the pulsar in the TeV binary PSR B1259-63/LS 2883, using 3-D SPH simulations of the tidal and wind interactions in this Be-pulsar system.
Hayasaki, Kimitake +6 more
core +1 more source
Pulsar Signal Adaptive Surrogate Modeling
AerospaceAs the number of spacecraft heading beyond Earth’s orbit increased in recent years, autonomous navigation solutions have become increasingly important. One such solution is pulsar-based navigation.
Tomáš Kašpárek, Peter Chudý
doaj +1 more source
Binary Pulsar Distances and Velocities from Gaia Data Release 2 [PDF]
Astrophysical Journal, 2018 The second data release from the Gaia mission (Gaia DR2) includes, among its billion entries, astrometric parameters for binary companions to a number of known pulsars, including white dwarf companions to millisecond pulsars (MSPs) and the non-degenerate
R. Jennings +4 more
semanticscholar +1 more source
The Kinematics of Pulsars [PDF]
Symposium - International Astronomical Union, 1985 Pulsars have a galactic radial distribution similar to that of many galactic populations such as HII regions, massive stars and supernova remnants. However they are generally much further from the plane of the Galaxy than these objects. Proper motion measurements sho that this is because they are typically moving with high velocities.
openaire +2 more sources
Electrodynamics of Pulsar Magnetospheres [PDF]
Space Science Reviews, 2016 31 pages, 11 figures, Accepted for publication in Space Science Reviews. Chapter in ISSI book on "Jets and Winds in Pulsar Wind Nebulae and Gamma-ray Bursts"
Cerutti, Benoît, Beloborodov, Andrei
openaire +5 more sources
A Perspective of Multi‐Reflecting TOF MS
Mass Spectrometry Reviews, EarlyView.ABSTRACT Time‐of‐flight mass spectrometry (TOF MS) excels in rapid and high‐sensitivity analysis, making it a cornerstone of analytical chemistry. But as sample complexity explodes in omics studies, so does the need for higher resolving power to ensure accurate results.
A. N. Verenchikov +3 more
wiley +1 more source
Does Pulsar B1757--24 Have a Fallback Disk?
, 2000 Radio pulsars are thought to spin-down primarily due to torque from magnetic dipole radiation (MDR) emitted by the time-varying stellar magnetic field as the star rotates.
Caswell J. L. +9 more
core +1 more source
The Double Pulsar Eclipses I: Phenomenology and Multi-frequency Analysis [PDF]
, 2012 The double pulsar PSR J0737-3039A/B displays short, 30 s eclipses that arise around conjunction when the radio waves emitted by pulsar A are absorbed as they propagate through the magnetosphere of its companion pulsar B.
A. Possenti +22 more
core +3 more sources