Results 91 to 100 of about 2,637 (230)
4U 1626-67 - A prograde spinning X-ray pulsar in a 2500 S binary system [PDF]
J. Middleditch+3 more
openalex +1 more source
An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers. [PDF]
Pang PTH+20 more
europepmc +1 more source
Discovery of a pulsar in a binary system
We have detected a pulsar with a pulsation period that varies systematically between 0.058967 and 0.059045 sec over a cycle of 0.3230 d. Approximately 200 independent observations over 5-minute intervals have yielded a well-sampled velocity curve which implies a binary orbit with projected semimajor axis sin i = 1.0 solar radius, eccentricity e = 0.615,
J. H. Taylor, R. A. Hulse
openaire +2 more sources
Can Slow Pulsars in Milky Way Globular Clusters Form via Partial Recycling?
Alongside the population of several hundred radio millisecond pulsars currently known in Milky Way globular clusters, a subset of six slowly spinning pulsars (spin periods 0.3–4 s) are also observed.
Kyle Kremer+5 more
doaj +1 more source
Binary Star Database: Binaries Discovered in Non-Optical Bands
The Binary star Database (BDB) is the world’s principal database of binary and multiple systems of all observational types. In particular, it should contain data on binaries discovered in non-optical bands, X-ray binaries (XRBs) and radio pulsars in ...
Malkov Oleg Yu.+2 more
doaj +1 more source
Strongly interacting matter exhibits deconfined behavior in massive neutron stars. [PDF]
Annala E+6 more
europepmc +1 more source
Recovering Pulsar Periodicity from Time-of-arrival Data by Finding the Shortest Vector in a Lattice
The strict periodicity of pulsars is one of the primary ways through which their nature and environment can be studied, and it has also enabled precision tests of general relativity and studies of nanohertz gravitational waves using pulsar timing arrays (
Dotan Gazith+2 more
doaj +1 more source