Results 271 to 280 of about 97,045 (300)
Study on the Horizontal Bearing Characteristic of a New Type of Offshore Rubber Airbag Branch Pile
Sustainability, 2022 In this work, a new type of marine rubber airbag branch pile has been presented, and the influences of the exposed length L0 of the pile, size of rubber airbag branch and depth S0 of rubber airbag branch embedded in soil on the horizontal bearing ...
Changfeng Yuan
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MORGOTH: incorporating horizontal branch modelling into star formation history determinations [PDF]
Monthly Notices of the Royal Astronomical Society, 2018 We present a new method that incorporates the horizontal branch morphology into synthetic colour-magnitude diagram based star formation history determinations.
Alessandro Savino +2 more
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Horizontal Branch of the Supraorbital Nerve and Temporal Branch of the Facial Nerve
Journal of Craniofacial Surgery, 2005The aim of this article is to describe anatomical detail of the course and territory of the horizontal branch of the supraorbital nerve, which connects with temporal branch of the facial nerve. Eighteen hemifaces of Korean cadavers (11 male, 7 female) fixed in 10% formaldehyde solution were dissected.
Kun, Hwang +4 more
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Astrophysics and Space Science, 1969
Evolutionary tracks of 0.9M ⊙, 0.7M ⊙ and 0.6M ⊙ models for Population II stars have been computed in the post-red giant phase. The stars are initially composed of a helium core containing a mass fraction equal to 0.9 and of a hydrogen-rich envelope.
V. Castellani, P. Giannone, A. Renzini
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Evolutionary tracks of 0.9M ⊙, 0.7M ⊙ and 0.6M ⊙ models for Population II stars have been computed in the post-red giant phase. The stars are initially composed of a helium core containing a mass fraction equal to 0.9 and of a hydrogen-rich envelope.
V. Castellani, P. Giannone, A. Renzini
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Low-mass evolution from he ignition to beyond the horizontal branch [PDF]
Space Science Reviews, 1980 The evolution of an 0.6 M/sub solar mass/ stellar model during core helium burning is presented. Following the off-center ignition of helium in the core flash, the star remains on the red giant branch for > 10/sup 6/ years, undergoing twelve additional ...
Despain, K.
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SPE Journal, 2012
Summary Horizontal and multibranch wells are likely to become the major means of modern exploitation strategies; inflow performances for these wells are needed. Because this paper considers the finite conductivity of a horizontal well, it establishes the inflow performance relationships (IPRs) for different branch configurations of ...
Huiqing Liu +3 more
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Summary Horizontal and multibranch wells are likely to become the major means of modern exploitation strategies; inflow performances for these wells are needed. Because this paper considers the finite conductivity of a horizontal well, it establishes the inflow performance relationships (IPRs) for different branch configurations of ...
Huiqing Liu +3 more
openaire +1 more source
A-Type Horizontal-Branch Stars
1975Horizontal-branch stars have attracted our attention as conspicuous examples of highly evolved population-II stars. Recent developments in the theoretical calculations of the internal structure of horizontal-branch stars (see Rood, 1970; Demarque and Mengel, 1971; Sweigart and Demarque, 1972) enable detailed studies on the evolutionary tracks ...
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Clean catalogues of blue horizontal-branch stars using Gaia EDR3
Astronomy and Astrophysics, 2021R Culpan, Íngrid Pelisoli, S Geier
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