Results 71 to 80 of about 8,519,684 (295)
Neutrino Background from Population III Stars
, 2011 Population III Stars (PopIII) are the first generation of stars formed from the collapse of the very first structures in the Universe. Their peculiar chemical composition (metal-free, resembling the Primordial Nucleosynthesis yields) affects their ...
Iocco F.
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Detection of isolated population III stars with the James Webb Space Telescope [PDF]
, 2013 The first Population III stars are predicted to form in minihaloes at z≈10-30. The JamesWebb Space Telescope (JWST), tentatively scheduled for launch in 2018, will probably be able to detect some of the first galaxies, but whether it will also be able to
Rydberg, Claes-Erik, +6 more
core +1 more source
How Population III Supernovae Determined the Properties of the First Galaxies
The Astrophysical JournalMassive Population III stars can die as energetic supernovae that enrich the early Universe with metals and determine the properties of the first galaxies.
Ke-Jung Chen +6 more
doaj +1 more source
Populations of rotating stars [PDF]
Astronomy & Astrophysics, 2014 16 pages, 16 figures, accepted for publication in A& ...
Georgy +8 more
openaire +3 more sources
Therapeutic Apheresis and Dialysis, EarlyView.ABSTRACT Background Maintenance hemodialysis (MHD) patients frequently suffer from frailty, characterized by reduced physical function and poor prognosis. Myokines, such as myonectin, secreted by muscle, are emerging regulators of systemic health. This study investigated the relationship between serum myonectin, adipokines (adiponectin, omentin), and ...
Kenichi Kono +7 more
wiley +1 more source
Radial-velocity measurements of subdwarf B stars [PDF]
, 2011 Subdwarf B (sdB) stars are hot, subluminous stars which are thought to be core-helium burning with thin hydrogen envelopes. The mechanism by which these stars lose their envelopes has been controversial, but it has been argued that binary star ...
Copperwheat, CM +14 more
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Carbon measurements in two ultra-faint dwarf galaxies: Grus II and Tucana IV
Astronomy & AstrophysicsThe ultra-faint dwarf galaxies (UFDs) are some of the oldest and most metal-poor environments in the Local Group. In particular, they are predicted to host the first stars (only H and He) that lit up in our Universe.
Verdiani Valentina +9 more
doaj +1 more source
The light from Population III stars [PDF]
Monthly Notices of the Royal Astronomical Society, 1986 Les etoiles de population III sont considerees comme une premiere generation d'etoiles pregalactiques ou pouvant etre presentes dans les jeunes galaxies.
openaire +1 more source
Cosmic reionization by stellar sources: population III stars [PDF]
Monthly Notices of the Royal Astronomical Society, 2004 40 pages, 9 ...
Sokasian, Aaron +4 more
openaire +5 more sources
Therapeutic Apheresis and Dialysis, EarlyView.ABSTRACT Background Chronic micro‐inflammation in patients with end‐stage renal disease (ESRD) is a significant driver of cardiovascular complications and diminished quality of life. While standard hemodialysis (SHD) effectively manages small‐molecule clearance, its ability to remove medium‐to‐large uremic toxins—the primary catalysts of systemic ...
Hongwei Zuo +5 more
wiley +1 more source