Results 31 to 40 of about 1,006,206 (194)

Spatial and Binary Parameter Distributions of Black Hole Binaries in the Milky Way Detectable with Gaia

open access: yesThe Astrophysical Journal, 2023
Soon after Gaia Data Release 3 (DR3) in 2022 June, some candidates (and one confirmed) of detached black hole (BH)–luminous companion (LC) binaries have been reported.
Minori Shikauchi   +3 more
doaj   +1 more source

The magnetosphere of the close accreting PMS binary V4046 Sgr [PDF]

open access: yes, 2014
SGG acknowledges support from the Science & Technology Facilities Council (STFC) via an Ernest Rutherford Fellowship [ST/J003255/1]. GAW is supported by a Discovery Grant from the Natural Science & Engineering Research Council of Canada (NSERC).V4046 ...
Damiani, F.   +78 more
core   +1 more source

Orbital Elements of visual binary stars with very short arcs: With application to double stars from the 1829 southern double star catalog of James Dunlop [PDF]

open access: yes, 2022
Binary double stars are those whose binding energies are less than zero. Obtaining binary star orbits from short arcs has been a long-standing problem in astrophysics.
Roderick R. Letchford   +5 more
core   +1 more source

Modelling and observations of molecules in discs around young stars [PDF]

open access: yes, 2013
This thesis contains a study of molecules within circumstellar discs around young stars. Firstly, the chemistry of a disc around a young, Class 0 protostar is modelled.
Ilee, John David
core   +6 more sources

Astrometric-Spectroscopic Determination of the Absolute Masses of the HgMn Binary Star φ Herculis [PDF]

open access: yesThe Astronomical Journal, 2007
The Mercury-Manganese star Phi Her is a well known spectroscopic binary that has been the subject of a recent study by Zavala et al. (2006), in which they resolved the companion using long-baseline interferometry. The total mass of the binary is now fairly well established, but the combination of the spectroscopy with the astrometry has not resulted in
openaire   +2 more sources

A spectro-astrometric study of southern pre-main sequence stars [PDF]

open access: yesAstronomy & Astrophysics, 2002
We present spectro-astrometric observations for 28 southern pre-main sequence (PMS) stars and investigate their circumstellar environment down to AU scales. The structures detected in the ``position spectra'' include: (1) almost all the known binary companions in our sample (Sz 68, Sz 41, HO Lup, VW Cha, S CrA, AS 205), (2) companion candidates which ...
Takami, Michihiro   +2 more
openaire   +3 more sources

The New Version of the Binary Star Database (BDB)

open access: yesOpen Astronomy, 2012
The Binary star database contains data on about 100 000 stellar systems of multiplicity 2 to 22, taken from a large variety of published catalogues for all types of binary stars: visual, orbital, astrometric, interferometric, spectroscopic, photometric ...
Kaygorodov P.   +4 more
doaj   +1 more source

Hidden Companions to Intermediate-mass Stars. IV. Uncovering a 1.1 M ⊙, 1.3 au Companion in the Astrometric Binary HIP 77541*

open access: yesResearch Notes of the AAS, 2023
Abstract There are many Hipparcos/Gaia astrometric binaries for which the nature of the companion is not known. Optical/near-infrared inteferometry is arguably the most efficient method to unambiguously identify such companions. Here we report on a VLTI/GRAVITY observation in which we detected a companion to the nearby astrometric binary
Idel Waisberg, Ygal Klein, Boaz Katz
openaire   +1 more source

Identifying Companions in Pulsar Binary Systems via Gaia Data

open access: yesUniverse
In the optical band, very few pulsars can be directly detected, but some of the pulsar binary companions can be observed. This study leverages high-precision astrometric data from Gaia Data Release 3 (DR3) to identify pulsar companions in binary systems.
Yueqi Song   +5 more
doaj   +1 more source

The GAPS programme at TNG

open access: yesAstronomy & Astrophysics
Context. The astrometric measurements provided by the Gaia space mission represent a key advancement in the search for and characterisation of exoplanets, helping in particular to solve the mass degeneracy intrinsic to the radial velocity (RV) method ...
Barbato D.   +24 more
doaj   +1 more source

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