Results 71 to 80 of about 260 (145)
Evidence for an Accretion Bridge in the DX Cha Circumbinary System from VLTI/MATISSE Observations
DX Cha (HD 104237) is a spectroscopic binary consisting of a Herbig A7.5Ve–A8Ve primary star and a K3-type companion. Here we report on new 3.55 μ m interferometric observations of this source with the Multi Aperture Mid-Infrared Spectroscopic Experiment
Tímea Juhász +22 more
doaj +1 more source
There is a clear dearth of very eccentric binaries among those for which individual eccentricities can be measured. In this paper we report on observations of the two nearby, bright and very eccentric visual binaries Zeta Bo\"otis ($\zeta$ Boo) and Eta ...
Idel Waisberg, Ygal Klein, Boaz Katz
doaj +1 more source
The Triple System V1371 Tau: An Eclipsing Binary with an Outer Be Star
Although triple systems are common, their orbital dynamics and stellar evolution remain poorly understood. We investigated the V1371 Tau system using TESS photometry, multiepoch spectroscopy, and recent interferometric data, confirming it as a rare ...
Danilo F. Rocha +12 more
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ANAorb: A robust framework for the optimal modelling of binaries
Context. Reliable orbital solutions for binary stars are essential for deriving accurate stellar parameters and for testing stellar-evolution models. However, current fitting approaches often struggle with local minima, strong parameter correlations, and
Andrade Manuel
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δ Circini: A massive hierarchical triple system with an eclipsing binary
δ Circini is known to be a massive multiple system containing a 3.9 d inner eclipsing binary in a slightly elliptical orbit exhibiting slow apsidal motion and a distant tertiary with a probable period of 1644 d.
Švrčková J. +8 more
doaj +1 more source
Time-lapse Very Long Baseline Interferometry Imaging of the Close Active Binary HR 1099
We report multiepoch astrometric very long baseline interferometry observations of the chromospherically active binary HR 1099 (V711 Tau, HD 22468) at six epochs over 63 days using the Very Long Baseline Array at 22.2 GHz.
Walter W. Golay +2 more
doaj +1 more source
Context. While massive stars are frequently found in triple architectures, the lack of observed parameter distributions has long remained a bottleneck for statistical models of their evolution. Aims.
Bordier E. +11 more
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Context. The fate of massive stars during the latest stages of their evolution is highly dependent on their mass-loss rate and geometry. The geometry of the mass-loss process can be inferred from the shape of the circumstellar material, which has a ...
Koumpia E. +14 more
doaj +1 more source
Chemical Fingerprints of M Dwarfs: High-resolution Spectroscopy on 31 M Dwarfs with SPIRou
We extend the methodology introduced by F. Jahandar et al. to determine the effective temperature and chemical abundances of 31 slowly rotating solar neighborhood M dwarfs (M1–M5) using high-resolution spectra from CFHT/SPIRou.
Farbod Jahandar +12 more
doaj +1 more source
Optical quantum super-resolution imaging and hypothesis testing. [PDF]
Zanforlin U +5 more
europepmc +1 more source

