Results 261 to 270 of about 2,677,677 (287)

Anti-Müllerian hormone levels and live birth rate in polycystic ovary syndrome patients undergoing assisted reproductive technology: a systematic review and meta-analysis. [PDF]

Front Med (Lausanne)
Wei X, Wang Y, Hu T, Li H, Liu L, Li Z, Zhao X.   +6 more
europepmc   +1 more source

Vapor-mediated wetting and imbibition control on micropatterned surfaces. [PDF]

Proc Natl Acad Sci U S A
Xu Z, Saiseau R, Ramírez-Soto O, Karpitschka S.   +3 more
europepmc   +1 more source

Viviendo entre dos culturas: Evaluating the psychometric properties of the Psychological Acculturation Scale among Latinx caregivers. [PDF]

PLoS One
Vázquez AL, Navarro Flores CM, Mendez L, Coleman J, Nagy GA, Garcia A, Domenech Rodríguez MM.   +6 more
europepmc   +1 more source

A Phase III triple-blind randomised placebo-controlled trial to evaluate effectiveness of early treatment with pregabalin to reduce pain severity after whiplash road traffic injury: study protocol for the PRioRTI Trial {1}. [PDF]

Trials
Sterling M, Farrell SF, Ferguson L, Mitchell G, Schug S, Ware RS, Dinh M, Celenza A, Connelly L, Hodges PW, Klyne DM, Elphinston R, Nikles J, McAuley J, Lin CC.   +14 more
europepmc   +1 more source

Close-in companions to contact binary stars

EAS Publications Series, 2013
W UMa-type contact binaries are composed of two late-type main-sequence stars, where both components are filling their critical Roche Lobes and sharing a common convective envelope. Their formation and evolution are unsolved problems in stellar astrophysics. This kind of binary systems have the lowest angular momentum and shortest orbital periods among
S.B. Qian, L.Y. Zhu, M. Zejda, Z. Mikulášek, J.J. Wang, N.P. Liu   +5 more
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Contact Tracing of Massive Binary Stars

Proceedings of the International Astronomical Union, 2022
AbstractStellar mergers produce more massive, rejuvenated (strongly magnetic) stars, with potentially peculiar properties, and can be detected as luminous red novae. Using a grid of detailed 1D binary evolution models, we aim to determine which binary systems are likely to merge and at what evolutionary stage.
Jan Henneco, Fabian R. N. Schneider, Saskia Hekker, Eva Laplace   +3 more
openaire   +1 more source

The evolutionary state of contact and near-contact binary stars

Monthly Notices of the Royal Astronomical Society, 1988
Calcul des masses, rayons et luminosites des composantes de 31 systemes binaires de type F-K proches ou en ...
R. W. Hilditch, D. J. King, T. M. McFarlane   +2 more
openaire   +1 more source

Multiplicity of Contact Binary Stars

2007
We present results of a preliminary investigation of triple star incidence for contact binary stars. The goal is to shed light on the possible role of distant companions which may have acquired and/or absorbed AM during evolution of multiple systems facilitating or enabling formation of contact binaries.
T. Pribulla, S.M. Rucinski
openaire   +1 more source