Results 41 to 50 of about 1,859,132 (364)

Clean catalogues of blue horizontal-branch stars using Gaia EDR3 [PDF]

open access: yesA&A 654, A107 (2021), 2021
Context: Blue horizontal-branch stars are very old objects that can be used as markers in studies of the Galactic structure and formation history. To create a clean sky catalogue of blue horizontal-branch stars, we cross-matched the Gaia data release 2 (DR2) dataset with existing reference catalogues to define selection criteria based on Gaia DR2 ...
arxiv   +1 more source

Person Re‐identification Based on Feature Erasure and Diverse Feature Learning

open access: yesIET Computer Vision, 2022
Robust and comprehensive modelling of targets is the key to successful person re‐identification. However, some useful information may be ignored, since CNNs tend to learn from the most distinctive feature region of the human body. In the present study, a
Lu Peng   +4 more
doaj   +1 more source

Numerical Simulation of Natural Gas Hydrate Exploitation in Complex Structure Wells: Productivity Improvement Analysis

open access: yesMathematics, 2021
About 90% of the world’s natural gas hydrates (NGH) exist in deep-sea formations, a new energy source with great potential for exploitation. There is distance from the threshold of commercial exploitation based on the single well currently used.
Hongyu Ye, Xuezhen Wu, Dayong Li
doaj   +1 more source

CHRONOGRAPHY OF THE MILKY WAY’S HALO SYSTEM WITH FIELD BLUE HORIZONTAL-BRANCH STARS [PDF]

open access: yes, 2015
In a pioneering effort, Preston et al. reported that the colors of blue horizontal-branch (BHB) stars in the halo of the Galaxy shift with distance, from regions near the Galactic center to about 12 kpc away, and interpreted this as a correlated ...
Rafael M. Santucci   +8 more
semanticscholar   +1 more source

Characterizing Fabric Anisotropy of Air-Pluviated Sands [PDF]

open access: yesE3S Web of Conferences, 2019
Sand particles depositing through air generally align their largest dimensions in horizontal plane, forming a cross anisotropic fabric. Therefore, sands display varying strength, permeability, compressibility with directions.
Sun Quan   +3 more
doaj   +1 more source

Metallicities of Globular Clusters m3 and m5 from VI CCD Photometry [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2000
To derive the metallicities of M3 and M5, we used the shape of red giant branch, horizontal branch magnitude, and red giant branch bump on the (V - I) - V color magnitude diagrams.
Young-Jong Sohn, Hyun-Chul Lee
doaj   +2 more sources

Meet the family − the catalog of known hot subdwarf stars

open access: yesOpen Astronomy, 2017
In preparation for the upcoming all-sky data releases of the Gaia mission, we compiled a catalog of known hot subdwarf stars and candidates drawn from the literature and yet unpublished databases.
Geier Stephan   +8 more
doaj   +2 more sources

Revisiting the variable star population in NGC 6229 and the structure of the horizontal branch [PDF]

open access: yes, 2015
We report an analysis of new $V$ and $I$ CCD time-series photometry of the distant globular cluster NGC 6229. The principal aims were to explore the field of the cluster in search of new variables, and to Fourier decompose the RR Lyrae light curves in ...
A. Ferro   +7 more
semanticscholar   +1 more source

The strange hot horizontal-branch binary star in NGC 6752

open access: yesOpen Astronomy, 2018
M5865 is the only so-far confirmed close binary found in the extreme horizontal branch (EHB) of a globular cluster. A detailed study has recently proposed that this object could be a close system (period P=1.61 days) comprising a EHB and a main-sequence ...
Bidin Christian Moni
doaj   +1 more source

The Na-O anticorrelation in horizontal branch stars. V. NGC 6723 [PDF]

open access: yes, 2014
We used FLAMES+GIRAFFE (Medusa mode) at the VLT to obtain moderately high resolution spectra for 30 red horizontal branch (RHB) stars, 4 RR Lyrae variables, and 17 blue horizontal branch (BHB) stars in the low-concentration, moderately metal-rich ...
R. Gratton   +9 more
semanticscholar   +1 more source

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