Results 41 to 50 of about 11,210,903 (298)
Evolution and Nucleosynthesis of Primordial Low‐Mass Stars
We discuss in detail the evolutionary properties of low mass stars M< 1 M(Solar) having metallicity lower than Z=10^(-6) from the pre- main sequence up to (almost) the end of the Asymptotic Giant Branch phase. We also discuss the possibility that the large [C,N/Fe] observed on the surface of the most Iron poor star presently known, HE0107-5240, may ...
I. PICARDI +7 more
openaire +5 more sources
By using direct N -body numerical simulations, we model the dynamical coevolution of two supermassive black holes (SMBHs) and the surrounding stars in merging galaxies. In order to investigate how different stellar components evolve during the merger, we
Shuo Li +5 more
doaj +1 more source
The accretion/ejection paradigm of low mass stars tested with HST [PDF]
Low-mass stars and brown dwarfs: IMF, accretion and activity ,Volterra, Italy, 17-20 October 2004In the last few years new investigation techniques have allowed us to study in depth the spectacular phenomenon of protostellar jets, and to test the ...
Coffey, Deirdre +4 more
core +1 more source
Facing the phase: Gravity-mode offset and buoyancy glitches in stars on the red-giant branch
Context. With the increasing precision of asteroseismic observations, it becomes possible to reliably measure oscillation properties of an increasing number of stars. Interpreting these measurements requires a good theoretical understanding of their link
van Lier T., Müller J., Hekker S.
doaj +1 more source
Zooming in on Individual Star Formation: Low- and High-Mass Stars [PDF]
Star formation is a multi-scale, multi-physics problem ranging from the size scale of molecular clouds ($\sim$10s pc) down to the size scales of dense prestellar cores ($\sim$0.1 pc) that are the birth sites of stars. Several physical processes like turbulence, magnetic fields and stellar feedback, such as radiation pressure and outflows, are more or ...
Anna L. Rosen +5 more
openaire +2 more sources
ABSTRACT Pediatric gastroenteropancreatic neuroendocrine neoplasms (GEP‐NENs) are extremely rare and clinically heterogeneous. Management has largely been extrapolated from adult practice. This European Standard Clinical Practice Guideline (ESCP), developed by the EXPeRT network in collaboration with adult NEN experts, provides (adult) evidence ...
Michaela Kuhlen +23 more
wiley +1 more source
The mass-radius relationship for very low mass stars: Four new discoveries from the HATSouth Survey [PDF]
We report the discovery of four transiting F-M binary systems with companions between 0.1 and 0.2 M☉ in mass by the HATSouth survey. These systems have been characterized via a global analysis of the HATSouth discovery data, combined with high-resolution
Schmidt, B +60 more
core +1 more source
A deep HST view of the open cluster NGC2158: Binaries, mass functions, and M-dwarf discontinuity
A significant fraction of stars in both the Galactic field and stellar clusters belong to binary systems. Understanding their properties is therefore fundamental for a comprehensive picture of stellar structure, stellar evolution, and cluster dynamics ...
Marchuk A. V. +15 more
doaj +1 more source
Solid Pseudopapillary Neoplasm of the Pancreas in Children and Adolescents: Expert Recommendations
ABSTRACT Solid pseudopapillary neoplasm of the pancreas (SPN) is a rare low‐grade malignant exocrine pancreatic tumor, mostly discovered during the second decade of life in females, with a very good prognosis, provided microscopically complete surgical excision is achieved.
Sabine Irtan +18 more
wiley +1 more source
Mass-radius relation of low and very low-mass stars revisited with the VLTI [PDF]
International audienceWe measured the radii of 7 low and very low-mass stars using long baseline interferometry with the VLTI interferometer and its VINCI and AMBER near-infrared recombiners.
Benisty, M. +29 more
core +1 more source

