Results 81 to 90 of about 165 (125)
First Detection of CH3OD in Prestellar Cores
The isotopic ratios of deuterated methanol derived around protostars are commonly used to infer the physical conditions under which they formed in the earlier prestellar stage.
Beatrice M. Kulterer +8 more
doaj +1 more source
Innovative approach for modelling gravity-induced signal path variations of VLBI radio telescopes
Gravitationally induced deformation of the receiving unit of radio telescopes used for Very Long Baseline Interferometry (VLBI) distorts the observations and biases the deduced products.
Michael Lösler +4 more
doaj +1 more source
Context. Recent Very Long Baseline Interferometry (VLBI) and Gaia astrometry reveal systematic milliarcsecond-scale offsets between the radio and optical centroids of active galactic nuclei (AGNs).
Fichet de Clairfontaine G. +3 more
doaj +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Fermi Unassociated Sources in the MeerKAT Absorption Line Survey
Over 2000 γ -ray sources identified by the Large Area Telescope on NASA's Fermi Gamma-ray Space Telescope are considered unassociated, meaning that they have no known counterparts in any other frequency regime.
Morgan Himes +10 more
doaj +1 more source
Using very long baseline interferometry data for the sources that comprise the third International Celestial Reference Frame (ICRF3), we examine the quality of the formal source-position uncertainties of ICRF3 by determining the excess astrometric ...
Phil Cigan +5 more
doaj +1 more source
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
Precise Mass, Orbital Motion, and Stellar Properties of the M-dwarf Binary LP 349−25AB
LP 349−25 is a well-studied close stellar binary system comprised of two late M dwarf stars, where both stars are close to the limit between star and brown dwarf. This system was previously identified as a source of gigahertz radio emission.
Salvador Curiel +3 more
doaj +1 more source
Astrometry with the 5-km Radio Telescope [PDF]
M. Ryle, B. Elsmore
openaire +1 more source
Main-oval Auroral Emission from a T6 Brown Dwarf: Observations, Modeling, and Astrometry
From a series of 5 GHz Very Long Baseline Array (VLBA) radio observations taken over a 1 yr span, we present the detection of compact, highly polarized radio emission from the T6 brown dwarf WISE J112254.72+255022.2, compatible with electron cyclotron ...
J. C. Guirado +5 more
doaj +1 more source

