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Mostrando ítems 1-10 de 11
Chemically tagging the Hyades stream: does it partly originate from the Hyades cluster?
(WILEY-BLACKWELL, 2011)
The Hyades stream has long been thought to be a dispersed vestige of the Hyades cluster. However, recent analyses of the parallax distribution, of the mass function, and of the action-space distribution of stream stars ...
Search for giant planets around seven white dwarfs in the Hyades cluster with the Hubble Space Telescope
(Oxford University Press, 2021-01-01)
Only a small number of exoplanets have been identified in stellar cluster environments. We initiated a high angular resolution direct imaging search using the Hubble Space Telescope (HST) and its Near-Infrared Camera and ...
A new method for calculating the convergent point of a moving group
(EDP SCIENCES S ALES ULIS CEDEX A, 2012)
Context. Convergent point (CP) search methods are important tools for studying the kinematic properties of open clusters and young associations whose members share the same spatial motion. Aims. We present a new CP search ...
The hypothesis of the local supercloud and the nearby moving groups of stars
(Oxford University Press, 2016-03)
The velocity distribution of stars in the solar neighbourhood can be globally characterized by the presence of two stellar streams (I and II). Stream I contains kinematic substructures, named moving groups of stars, such ...
NGC2587: a sparse open cluster projected on to a populous star field
(Oxford University Press, 2009-07)
We present CCD photometry in the Johnson U, B and V and Kron–Cousins I passbands for the open cluster NGC 2587. The sample consists of 4406 stars reaching down to V∼ 21.0. We developed a new method to clean statistically ...
The extended main-sequence turn-off of the Milky Way open cluster Collinder 347
(Wiley Blackwell Publishing, Inc, 2019-10-07)
We made use of the Gaia DR2 archive to comprehensively study the Milky Way open cluster Collinder 347, known until now as a very young object of solar metal content. However, the G versus GBP − GRP colour-magnitude diagram ...
Observational templates of star cluster disruption - The stellar group NGC 1901 in front of the Large Magellanic Cloud
(2007)
Context. Observations indicate that present-day star formation in the Milky Way disk takes place in stellar ensembles or clusters rather than in isolation. Bound, long-lived stellar groups are known as open clusters. They ...