Results 221 to 230 of about 24,425 (256)
Gravitational wave content and stability of uniformly, rotating, triaxial neutron stars in general relativity. [PDF]
Phys Rev D, 2017 Tsokaros A +5 more
europepmc +1 more source
Insights into conscious cognitive information processing. [PDF]
Front Behav NeurosciDere E.
europepmc +1 more source
H.E.S.S.: Variable VHE gamma-Ray Emission from the Binary Pulsar PSR B1259-63
, 2005 S. Schlenker +4 more
openalex +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Nature, 1977
As X-ray astronomy enters the Einstein era when faint, distant, and exotic X-ray sources are being investigated, we thought it might be useful to review some of the progress made over the past decade on a class of relatively nearby objects that have contributed richly to our understanding of astrophysics — the binary X-ray pulsars.
S. Rappaport, P. C. Joss
openaire +1 more source
As X-ray astronomy enters the Einstein era when faint, distant, and exotic X-ray sources are being investigated, we thought it might be useful to review some of the progress made over the past decade on a class of relatively nearby objects that have contributed richly to our understanding of astrophysics — the binary X-ray pulsars.
S. Rappaport, P. C. Joss
openaire +1 more source
Navigation using binary pulsars
Science China Physics, Mechanics and Astronomy, 2012The issue of navigation using binary pulsars is investigated in this paper. We show how the effect of the binary motion is incorporated in the navigation measurement equation. Necessary reference systems and time scales are introduced and the transformation between different time scales is derived. Based mainly on Damour and Deruelle’s binary model and
LiangWei Huang +3 more
openaire +1 more source
2021
1967 wurde der erste Pulsar als scheinbar pulsierende Radioquelle entdeckt. Seitdem wurden mehr als 2800 weitere Pulsare gefunden, die meisten davon ebenfalls im Radiobereich. Mit dem Start des Fermi Gamma-ray Space Telescope im Jahr 2008 wurden mittlerweile mehr als 250 Gamma-Pulsare entdeckt.
openaire +1 more source
1967 wurde der erste Pulsar als scheinbar pulsierende Radioquelle entdeckt. Seitdem wurden mehr als 2800 weitere Pulsare gefunden, die meisten davon ebenfalls im Radiobereich. Mit dem Start des Fermi Gamma-ray Space Telescope im Jahr 2008 wurden mittlerweile mehr als 250 Gamma-Pulsare entdeckt.
openaire +1 more source
Nature, 1988
Tentative d'explication schematique de l'evolution des systemes binaires pouvant donner naissance a des pulsars tres ...
openaire +1 more source
Tentative d'explication schematique de l'evolution des systemes binaires pouvant donner naissance a des pulsars tres ...
openaire +1 more source
Nature, 1978
It is shown that binary systems containing moderately young pulsars may emit high-energy neutrinos (between 1 and 100 TeV) at detectable levels. The pulsars are assumed to have total luminosities of the order of 10 to the 38th erg/sec. The neutrinos are produced by high energy particles (e.g. protons) from the pulsar striking the companion.
openaire +1 more source
It is shown that binary systems containing moderately young pulsars may emit high-energy neutrinos (between 1 and 100 TeV) at detectable levels. The pulsars are assumed to have total luminosities of the order of 10 to the 38th erg/sec. The neutrinos are produced by high energy particles (e.g. protons) from the pulsar striking the companion.
openaire +1 more source
Binary and Millisecond Pulsars
2014The first evidence for neutron stars residing in binaries came in the early 60s when Giacconi et al. (1962) discovered the first extrasolar X-ray source, Sco X\(-\)1.
openaire +1 more source