Results 71 to 80 of about 11,697 (215)
Radio astrometry with chromatic AGN core positions [PDF]
Accepted for publication in Astronomy & Astrophysics, 4 ...
openaire +2 more sources
Abstract We present James Webb Space Telescope observations of the globular cluster NGC 6397 and use them to extend to infrared wavelengths the characterization of the cluster's entire white dwarf (WD) cooling sequence (CS). The data allows us to probe fundamental astrophysical WD properties and to search for evidence in their colors for (or against ...
L. R. Bedin +11 more
wiley +1 more source
A Radio Counterpart to a Jupiter-mass Binary Object in Orion
Using James Webb Space Telescope near-infrared data of the inner Orion Nebula, Pearson & McCaughrean detected 40 Jupiter-mass binary objects (JuMBOs).
Luis F. Rodríguez +2 more
doaj +1 more source
Not So Fast: A New Catalog of Meteor Persistent Trains
Abstract This paper presents the results of a nearly 2‐year long campaign to detect and analyze meteor persistent trains (PTs)—self‐emitting phenomena which can linger up to an hour after their parent meteor. The modern understanding of PTs has been primarily developed from the Leonid storms at the turn of the century; our goal was to assess the ...
L. E. Cordonnier +4 more
wiley +1 more source
A Study of Real-time Detection Methods for Solar Radio Burst Identification
Solar flares, coronal mass ejections, and other solar radio burst phenomena release substantial amounts of solar radiation energy, resulting in adverse space weather conditions and posing significant hazards in space. Spectrum analysis conducted manually
YongLin Yu +6 more
doaj +1 more source
Chandra astrometry sets a tight upper limit to the proper motion of SGR 1900+14
The soft gamma-ray repeater (SGR) SGR 1900+14 lies a few arcminutes outside the edge of the shell supernova remnant (SNR) G42.8+0.6. A physical association between the two systems has been proposed - for this and other SGR-SNR pairs - based on the ...
A. De Luca +24 more
core +1 more source
Pilot VLBI Survey of SiO v=3 J=1--0 Maser Emission around Evolved Stars [PDF]
In this Letter, we report detections of SiO v=3 J=1--0 maser emission in very long baseline interferometric (VLBI) observations towards 4 out of 12 long-period variable stars: WX Psc, R Leo, W Hya, and T Cep.
Cho, Se-Hyung +11 more
core +2 more sources
Astrometry and geodesy with radio interferometry: experiments, models, results [PDF]
83 pages, 19 Postscript figures. To be published in Rev. Mod. Phys., Vol.
Sovers, Ojars J. +2 more
openaire +2 more sources
The fireball of November 24, 1970, as the most probable source of the Ischgl meteorite
Abstract The discovery of the Ischgl meteorite unfolded in a captivating manner. In June 1976, a pristine meteorite stone weighing approximately 1 kg, fully covered with a fresh black fusion crust, was collected on a mountain road in the high‐altitude Alpine environment.
Maria Gritsevich +15 more
wiley +1 more source
The millisecond pulsar J1713+0747 underwent a sudden and significant pulse shape change between 2021 April 16 and 17 (MJDs 59320 and 59321). Subsequently, the pulse shape gradually recovered over the course of several months.
Ross J. Jennings +43 more
doaj +1 more source

