Results 21 to 30 of about 2,560 (288)
MOLECULAR CLOUD EVOLUTION. III. ACCRETION VERSUS STELLAR FEEDBACK [PDF]
We numerically investigate the effect of feedback from the ionizing radiation heating from massive stars on the evolution of giant molecular clouds (GMCs) and their star formation efficiency (SFE). We find that the star-forming regions within the GMCs are invariably formed by gravitational contraction.
Enrique Vázquez-Semadeni +4 more
openaire +2 more sources
Accretion‐powered Stellar Winds. III. Spin‐Equilibrium Solutions [PDF]
We compare the stellar wind torque calculated in a previous work (Paper II) to the spin-up and spin-down torques expected to arise from the magnetic interaction between a slowly rotating ($\sim 10$% of breakup) pre-main-sequence star and its accretion disk.
Matt, Sean P., Pudritz, Ralph E.
openaire +3 more sources
We perform three-dimensional (3D) magnetohydrodynamic simulations of magnetospheric accretion in a T Tauri star to study the accretion and wind structures in the close vicinity of the star.
Shinsuke Takasao +3 more
doaj +1 more source
Observable Signatures of Classical T Tauri Stars Accreting in an Unstable Regime
We discuss key observational signatures of Classical T Tauri stars (CTTSs) accreting through Rayleigh-Taylor instability, which occurs at the interface between an accretion disk and a stellar magnetosphere.
Kurosawa Ryuichi, Romanova M. M.
doaj +1 more source
SPIN EVOLUTION OF ACCRETING YOUNG STARS. II. EFFECT OF ACCRETION-POWERED STELLAR WINDS [PDF]
Accepted for publication in ApJ; 13 pages, 5 ...
P. Matt, Sean +3 more
openaire +3 more sources
The Auriga stellar haloes: connecting stellar population properties with accretion and merging history [PDF]
Accepted to MNRAS.
Antonela Monachesi +11 more
openaire +5 more sources
Accretion disks in luminous young stellar objects [PDF]
71 pages, 19 figures.
BELTRAN SOROLLA, MARIA TERESA +1 more
openaire +3 more sources
Mapping the evolution of mitochondrial complex I through structural variation
Respiratory complex I (CI) is crucial for bioenergetic metabolism in many prokaryotes and eukaryotes. It is composed of a conserved set of core subunits and additional accessory subunits that vary depending on the organism. Here, we categorize CI subunits from available structures to map the evolution of CI across eukaryotes. Respiratory complex I (CI)
Dong‐Woo Shin +2 more
wiley +1 more source
This work presents a study of the evolution of the stellar accretion rates of pre-main-sequence intermediate-mass stars. We compare the accretion rate of the younger intermediate-mass T Tauri stars (IMTTSs) with the older Herbig stars into which they ...
Sean D. Brittain +3 more
doaj +1 more source
Mergers of accreting stellar-mass black holes [PDF]
We present post-Newtonian $N$-body simulations on mergers of accreting stellar-mass black holes (BHs), where such general relativistic effects as the pericenter shift and gravitational wave (GW) emission are taken into consideration. The attention is concentrated on the effects of the dynamical friction and the Hoyle-Lyttleton mass accretion by ambient
Tagawa, Hiromichi +2 more
openaire +3 more sources

