Results 261 to 270 of about 301,814 (290)

Is radiofrequency ablation of renal cancer metastases a suitable alternative to surgical metastectomy: A systematic review. [PDF]

Ir J Med Sci
McNicholas DP, Dexter E, Hampson A, Evans J, Venugopal S.   +4 more
europepmc   +1 more source

Knowledge, attitudes, and behaviours related to reduced-sodium salt: a systematic review. [PDF]

J Hum Hypertens
Kissock KR, Ghammachi N, Hoek AC, Bullen JD, Webster J, Pettigrew S, Garg N, Neal B, Trieu K.   +8 more
europepmc   +1 more source

Mechanisms for stimulating facility quality improvement: A positive deviance study of Tanzania's Star Rating Assessment. [PDF]

PLOS Glob Public Health
Roder-DeWan S, Gage A, Shamba D, Rajab H, Somba M, Mohamed M, Ramesh M, Yahya T, Eliakimu E.   +8 more
europepmc   +1 more source

Acute Kidney Injury in Children with Polyuria: A Systematic Review. [PDF]

J Clin Med
Rivetti G, Braile M, Di Sessa A, Tirelli P, Guarino S, Miraglia Del Giudice E, Guzzo I, Marzuillo P.   +7 more
europepmc   +1 more source

Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab

Santos Ld, Owen J, Duvvuri G, Loyd ROP, Vidotto A, Presa A, Bourrier V, King G, Airapetian V, Ehrenreich D, France K, Lendl M, Lothringer J, Nielsen L.   +13 more
europepmc   +1 more source

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Survival of Population III stars

Proceedings of the International Astronomical Union, 2018
AbstractIn our earlier studyDutta (2016a), it has been shown that a number of primordial protostars (the ‘first stars’ in the Universe, also known as Population III or Pop III stars) are being ejected from the cluster of their origin with the velocity exceeding their escape velocity.
Jayanta Dutta, Sharanya Sur, Athena Stacy, Jasjeet Singh Bagla   +3 more
openaire   +1 more source

Observational manifestations of population III stars

Astrophysics, 1987
The thermal history of gas heated by explosions of population III stars at red shifts z approx. 100 is calculated. The distortions in the spectrum of the microwave radiation and the intensity of the resulting x rays are determined. Bounds on the energy release produced by the explosions of such stars are compared with available observations.
B. V. Vainer, V. V. Chuvenkov, Yu. A. Shchekinov   +2 more
openaire   +1 more source

GRAVITATIONAL COLLAPSE OF POPULATION III STARS

The Eleventh Marcel Grossmann Meeting, 2008
▌ The expected diffuse cosmic neutrino flux produced by Pop III stars during their nuclear burning and their core-collapse phases▌ Estimated flux is comparable to the diffuse neutrino fluxes produced by ordinary SNe. However, due to the large cosmological redshift, the typical energies are MeV and sub-MeV, where the other components dominate.
YUDAI SUWA, TOMOYA TAKIWAKI, KEI KOTAKE, KATSUHIKO SATO   +3 more
openaire   +1 more source

Nucleosynthesis in Aspherical Explosions of Population III Stars

AIP Conference Proceedings, 2008
We present the nucleosynthetic yields of Population III core‐collapse supernovae (SNe) focusing on the cases of hyper‐energetic (Hypernovae, HNe) and hyper‐aspherical (jet‐induced) explosions. We show that (1) the explosions with large energy deposition rate, Ėdep, are observed as GRB‐HNe and their yields can explain the abundances of normal extremely ...
Nomoto, K., Tominaga, N., Tanaka, M., Maeda, K., Umeda, H.   +4 more
openaire   +2 more sources

Nucleosynthetic Consequences of Population III Stars

1986
It is argued that the Population III stars with the most explanatory power are Very Massive Objects (VMOs) in the mass range ...
B. J. Carr, W. Glatzel
openaire   +1 more source