Results 41 to 50 of about 35,614 (300)

THE DESTRUCTION OF THIN STELLAR DISKS VIA COSMOLOGICALLY COMMON SATELLITE ACCRETION EVENTS [PDF]

open access: yesThe Astrophysical Journal, 2009
6 pages, 4 figures; accepted by ApJL; high-resolution version and example movie of simulation available at http://web.me.com/purcellgalaxies/workshop/log/Entries/2008/10/15_The_Destruction_of_thin_stellar_disks_via_cosmologically_common_mergers ...
Purcell, Chris W.   +2 more
openaire   +2 more sources

Migration of gap-opening planets in 3D stellar-irradiated accretion disks [PDF]

open access: yesAstronomy & Astrophysics, 2020
Context. The origin of giant planets at moderate separations ≃1–10 au is still not fully understood because numerical studies of Type II migration in protoplanetary disks often predict a decay of the semi-major axis that is too fast. According to recent 2D simulations, inward migration of a gap-opening planet can be slowed down or even reversed if the ...
O. Chrenko, D. Nesvorný
openaire   +2 more sources

LAMOST Reveals Long-lived Protoplanetary Disks

open access: yesThe Astronomical Journal
While both observations and theories demonstrate that protoplanetary disks are not expected to live much longer than ∼10 Myr, several examples of prolonged disks have been observed in the past.
Xiao-Long Wang   +4 more
doaj   +1 more source

Stellar wind accretion and accretion disk formation: Applications to neutron star high-mass X-ray binaries [PDF]

open access: yesPublications of the Astronomical Society of Japan, 2019
Abstract Recent X-ray observations have revealed the complexity and diversity of high-mass X-ray binaries (HMXBs). This diversity challenges a classical understanding of the accretion process on to the compact objects. In this study, we reinforce the conventional concept of the nature of wind-fed accretion on to a neutron star ...
Karino, Shigeyuki   +2 more
openaire   +2 more sources

Hyperosmotic stress induces PARP1‐mediated HPF1‐dependent mono(ADP‐ribosyl)ation

open access: yesFEBS Letters, EarlyView.
Sorbitol‐induced hyperosmotic stress rapidly induces reversible mono(ADP‐ribosyl)ation (MARylation) on PARP1 without the signs of genotoxic signaling. We show that PARP1 autoMARylation is HPF1 dependent and forms hydroxylamine‐resistant O‐glycosidic linkages.
Anna Georgina Kopasz   +11 more
wiley   +1 more source

Understanding Balmer Decrements in T Tauri Stars in Terms of Multiflow Magnetospheric Accretion

open access: yesThe Astrophysical Journal
Magnetospheric accretion is the paradigm for accretion in classical T Tauri stars (CTTSs). However, the standard, one-flow magnetospheric accretion model fails to replicate important characteristics such as the observed Balmer decrements. We address this
Naiara Patiño   +6 more
doaj   +1 more source

Cooling of young stars growing by disk accretion

open access: yes, 2007
In the initial formation stages young stars must acquire a significant fraction of their mass by accretion from a circumstellar disk that forms in the center of a collapsing protostellar cloud. Throughout this period mass accretion rates through the disk
Arras P.   +11 more
core   +1 more source

Disk-mediated accretion burst in a high-mass young stellar object [PDF]

open access: yesNature Physics, 2016
27 pages, 3 figures. Published in Nature Physics, 2016, Vol.
Caratti o Garatti, A   +15 more
openaire   +5 more sources

Tumour–host interactions in Drosophila: mechanisms in the tumour micro‐ and macroenvironment

open access: yesMolecular Oncology, EarlyView.
This review examines how tumour–host crosstalk takes place at multiple levels of biological organisation, from local cell competition and immune crosstalk to organism‐wide metabolic and physiological collapse. Here, we integrate findings from Drosophila melanogaster studies that reveal conserved mechanisms through which tumours hijack host systems to ...
José Teles‐Reis, Tor Erik Rusten
wiley   +1 more source

Secret of Longevity: Protoplanetary Disks as a Source of Gas in Debris Disks

open access: yesThe Astrophysical Journal
While protoplanetary disks (PPDs) are generally thought to disperse within several million years, recent observations have revealed gas in their older counterparts, debris disks.
Wataru Ooyama   +4 more
doaj   +1 more source

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