Results 121 to 130 of about 11,731 (215)
Interstellar comets provide rare opportunities for probing the diversity of refractory and volatile inventory around other stars. As the second ever interstellar comet and the third interstellar object, 3I/ATLAS has been the focus of telescopic ...
Juncen Li +3 more
doaj +1 more source
The high optical brightness of the BlueWalker 3 satellite. [PDF]
Nandakumar S +39 more
europepmc +1 more source
The Celestial Frame and the Weighting of the Celestial Pole Offsets in the Computation of VLBI-Based Corrections for the Main Lunisolar Nutation Terms. [PDF]
Puente V, Folgueira M.
europepmc +1 more source
From reference frames to relativistic experiments: Absolute and relative radio astrometry
25 pages, 7 figures--Presented at JENAM meeting in Budapest, 27-30 August ...
openaire +2 more sources
A VLBI Software Correlator for Fast Radio Transients
One major goal in fast radio burst science is to detect fast radio bursts (FRBs) over a wide field of view without sacrificing the angular resolution required to pinpoint them to their host galaxies.
Calvin Leung +16 more
doaj +1 more source
Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]
Caleb M +21 more
europepmc +1 more source
ABSTRACT The Gaia celestial reference frame (Gaia-CRF) will benefit from a close assessment with independent methods, such as Very Long Baseline Interferometry (VLBI) measurements of radio stars at bright magnitudes. However, obtaining full astrometric parameters for each radio star through VLBI measurements demands a significant amount ...
Jingdong Zhang +14 more
openaire +2 more sources
Dynamical Mass of the Ophiuchus Intermediate-mass Stellar System S1 with DYNAMO-VLBA
We report dynamical mass measurements of the individual stars in the most luminous and massive stellar member of the nearby Ophiuchus star-forming region, the young tight binary system S1.
Jazmín Ordóñez-Toro +10 more
doaj +1 more source
Probing a southern hemisphere VLBI Intensive baseline configuration for UT1 determination. [PDF]
Böhm S +8 more
europepmc +1 more source
Submillimeter Observations of the White Dwarf Pulsar AR Sco
AR Scorpii, the so-called white dwarf (WD) pulsar, contains a rapidly rotating magnetic WD ( P _spin = 117.0564 s) interacting with a cool, red dwarf (RD) companion in a 3.56 hr orbit. It is a strong radio source with an inverted spectral index between 1
Paul E. Barrett, Mark A. Gurwell
doaj +1 more source

