Results 41 to 50 of about 660,853 (292)
Tides and angular momentum redistribution inside low-mass stars hosting planets: a first dynamical model [PDF]
We introduce a general mathematical framework to model the internal transport of angular momentum in a star hosting a close-in planetary/stellar companion. By assuming that the tidal and rotational distortions are small and that the deposit/extraction of
Lanza, A. F., Mathis, S.
core +2 more sources
Direct evidence of a sub-stellar companion around CT Cha
In our ongoing search for close and faint companions around T Tauri stars, we found a very faint (Ks=14.9mag, Ks_0=14.4mag) object, just ~2.67" northwest of the Chamaeleon star-forming region member CT Cha corresponding to a projected separation of ...
A. Bedalov +91 more
core +1 more source
The identity of the progenitor systems of SNe Ia is still uncertain. In the single-degenerate (SD) scenario, the interaction between the SN blast wave and the outer layers of a main sequence (MS) companion star strips off H-rich material which is then ...
Edelmann, P. +7 more
core +1 more source
Detecting the Companions and Ellipsoidal Variations of RS CVn Primaries: I. sigma Geminorum [PDF]
To measure the properties of both components of the RS CVn binary sigma Geminorum (sigma Gem), we directly detect the faint companion, measure the orbit, obtain model-independent masses and evolutionary histories, detect ellipsoidal variations of the ...
Aarnio, Alicia N. +19 more
core +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
WIMP dark matter hidden behind its companion
The WIMP dark matter (DM) hypothesis now is in an awkward position, owing to the present strong exclusion from DM direct detection. In this article we design a mechanism to evade this constraint. The idea is simple.
Jun Guo, Zhaofeng Kang, Peng Zhang
doaj +1 more source
Giant planets are usually thought to form within a few tens of AU of their host stars, and hence it came as a surprise when we found what appeared to be a planetary mass (~0.008 Msun) companion around the 5 Myr-old solar mass star 1RXS J160929.1-210524 ...
Allard +36 more
core +1 more source
Companion eccentricity diffusion & multiple populations: the companion accretion model
Globular clusters exhibit abundance variations, defining ‘multiple populations’, which have prompted a protracted search for their origin since the 1970s. In this talk, I discuss a novel model to explain these variations, the 'companion accretion model'. An overlooked characterstic of the dynamical perturbation cross-section for binaries in hot stellar
openaire +1 more source
ABSTRACT Background Oral mucositis is a common and debilitating side effect of childhood cancer and stem cell transplant treatments. It affects the quality of life of children and young people (CYP) and places a strain on services. Photobiomodulation is recommended for oral mucositis prevention in international guidance but is poorly implemented in UK ...
Claudia Heggie +4 more
wiley +1 more source
Improved radial velocity orbit of the young binary brown dwarf candidate ChaHa8
The very young brown dwarf candidate ChaHa8 was recently discovered to have a close (~1AU) companion by means of radial velocity monitoring. We present additional radial velocity data obtained with UVES/VLT between 2007 and 2010, which significantly ...
A. Müller +20 more
core +1 more source

