Results 61 to 70 of about 16,047,641 (362)
Low-Mass Stars. II. The Core Mass--Luminosity Relations for Low-Mass Stars
The Astrophysical Journal, 1988 Etude de la relation masse-luminosite dans la litterature pour des etoiles de masse intermediaire, et extension a des etoiles de faible masse (0,8 M ○. -3 M ○. )
Arnold I. Boothroyd, I.-Juliana Sackmann
openaire +2 more sources
Journal of Materials Research and Technology, 2021 The microstructural and crystallographic features of the β phase in TNM alloy during the hot extrusion at 1290 °C and the subsequent cooling process were investigated. Except the original grain boundary β phase, two categories of β particles, along grain
Fengming Qiang +6 more
doaj
NEUTRON STAR MASS–RADIUS CONSTRAINTS OF THE QUIESCENT LOW-MASS X-RAY BINARIES X7 AND X5 IN THE GLOBULAR CLUSTER 47 TUC [PDF]
, 2016 We present Chandra/ACIS-S subarray observations of the quiescent neutron star (NS) low-mass X-ray binaries X7 and X5 in the globular cluster 47 Tuc.
S. Bogdanov +3 more
semanticscholar +1 more source
Management of Low Bone Mass in Female Athletes [PDF]
Kosin Medical Journal, 2014 As female athletic participation has increased, the positive effects of exercise on health have become evident. However, with this growth in sports activity, a set of health problems unique to the female athlete has emerged.
Hoon Choi
doaj +1 more source
Tracing Embedded Stellar Populations in Clusters and Galaxies using Molecular Emission: Methanol as a Signature of the Low-Mass End of the IMF [PDF]
, 2015 Most low-mass protostars form in clusters, in particular high-mass clusters; however, how low-mass stars form in high-mass clusters and what the mass distribution is, are still open questions both in our own Galaxy and elsewhere. To access the population of forming embedded low-mass protostars observationally, we propose to use molecular outflows as ...
arxiv +1 more source
Formation and composition of planets around very low mass stars [PDF]
, 2016 Context. The recent detection of planets around very low mass stars raises the question of the formation, composition, and potential habitability of these objects. Aims.
Y. Alibert, W. Benz
semanticscholar +1 more source
Symposium - International Astronomical Union, 1991 Recent results on low mass AGB stars are presented. Observed amounts of AGB mass loss imply that thermal pulses will only be encountered for stars of initial mass less than about 4M⊙ for Pop I and 3 M⊙ for Pop II. Mc – L, Me – τif, and Mc – Tb relations are summarized.
I. J. Sackmann, A. I. Boothroyd
openaire +2 more sources
The New Plastic Flow Machining Process for Producing Thin Sheets
Advances in Materials Science and Engineering, 2018 A new severe plastic deformation (SPD) process called plastic flow machining (PFM) was recently proposed to produce thin sheets with gradient structures.
Viet Q. Vu +3 more
doaj +1 more source
Emergence of Nonwhite Noise in Langevin Dynamics with Magnetic Lorentz Force [PDF]
Phys. Rev. E 97, 032117 (2018), 2017 We investigate the low mass limit of Langevin dynamics for a charged Brownian particle driven by the magnetic Lorentz force. In the low mass limit, velocity variables relaxing quickly are coarse-grained out to yield effective dynamics for position variables. Without Lorentz force, the low mass limit is equivalent to the high friction limit.
arxiv +1 more source
WHERE ARE THE LOW-MASS POPULATION III STARS? [PDF]
, 2016 We study the number and the distribution of low-mass Population III (Pop III) stars in the Milky Way. In our numerical model, hierarchical formation of dark matter minihalos and Milky-Way-sized halos are followed by a high-resolution cosmological ...
T. Ishiyama +5 more
semanticscholar +1 more source