Results 61 to 70 of about 1,006,206 (194)
Seismic inference of 57 stars using full-length Kepler data sets
We present stellar properties of 57 stars from a seismic inference using full-length data sets from Kepler (mass, age, radius, distances). These stars comprise active stars, planet-hosts, solar-analogs, and binary systems.
Creevey Orlagh +8 more
doaj +1 more source
Uncertainties in Historic Visual Double Star Measures—III Accurate Calibration Pairs
ABSTRACT Based on space‐based positions and proper motions, we present accurate rectilinear elements for 857 double star pairs over the celestial sphere. These elements allow for the computation of precision ephemeris Position Angles and Separations of these pairs.
Roderick R. Letchford, Graeme L. White
wiley +1 more source
ABSTRACT We present James Webb Space Telescope observations of M 4—the closest globular cluster—that probe the lower Main Sequence down to the hydrogen‐burning limit. The unveiled stellar sequence reaches much fainter luminosities than previously possible, revealing a few extremely red objects that are consistent with brown dwarfs as cool as Teff∼1000K$
L. R. Bedin +10 more
wiley +1 more source
Mass Transfer in Binary Stars using Smoothed Particle Hydrodynamics [PDF]
Despite numerous efforts to better understand binary star evolution, some aspects of it remain poorly constrained. In particular, the evolution of eccentric binaries has remained elusive mainly because the Roche lobe formalism derived for circular ...
Lajoie, Charles-Philippe
core
Photometry of Astrometric Reference Stars
We present, in the third in a series of papers, UBVRI, DDO, and uvby, Hβ photometry of astrometric reference stars. Spectral types and luminosity classifications made from the colors are used to determine their spectroscopic parallaxes.
Persinger, Tim +4 more
core +1 more source
Reassessing the Relationship Between Meteor Radio Afterglows and Optical Persistent Trains
Abstract Meteor radio afterglows (MRAs) and optical persistent trains (PTs) are two types of long‐lived phenomena which are occasionally observed following the occurrence of a meteor. Both phenomena are thought to be produced by intrinsic emission mechanisms; PTs have been associated with chemiluminescent reactions between meteoric metals and ...
L. E. Cordonnier +5 more
wiley +1 more source
We compiled a sample of 47 single-lined spectroscopic binaries (SB1s) with available relative astrometric measurements. By combining radial velocities, relative astrometry, and absolute astrometry when available and reliable, we determine the component ...
Xiaoli Wang, Fang Xia, Yanning Fu
doaj +1 more source
Weighing the Darkness. II. Astrometric Measurement of Partial Orbits with Gaia
Over the course of several years, stars trace helical trajectories as they traverse across the sky due to the combined effects of proper motion and parallax.
Jeff J. Andrews +4 more
doaj +1 more source
We present spectroscopic follow-up observations of binary systems from the Gaia Data Release 3 (DR3) binary catalog that were selected to have large enough mass functions for their companions to be black holes or neutron stars.
Joshua D. Simon +10 more
doaj +1 more source
ABSTRACT We present relative astrometric measurements of visual double stars, made in 2017–2018 with the speckle camera PISCO at the 1‐m Epsilon telescope of the C2PU facility (Observatoire de la Côte d'Azur, Calern site). Our observing list contains orbital couples as well as double stars whose motion is still uncertain.
M. Scardia +11 more
wiley +1 more source

