Zobrazeno 1 - 10
of 42
pro vyhledávání: '"Weishan, Zhu"'
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 2, p 141 (2024)
Large-scale cosmic filaments may have played an important role in shaping the properties of galaxies. Meanwhile, cosmic filaments are believed to harbor a substantial portion of the missing baryons at redshift z < 2. To inspect the role of filaments
Externí odkaz:
https://doaj.org/article/5ca48b99784f48baba4c53d410084c28
Publikováno v:
BMJ Open, Vol 13, Iss 5 (2023)
Introduction Technological advances are changing nursing practice; however, nurse-led virtual care for chronic disease management has not yet been adequately explored and described. This study will review and analyse the effects of nurse-led virtual
Externí odkaz:
https://doaj.org/article/5574a8b8ae7a49c6aa1673a58dcd62f4
Publikováno v:
Universe, Vol 8, Iss 10, p 535 (2022)
Probing the polarization of gravitational waves (GWs) would provide evidence of graviton, indicating the quantization of gravity. Motivated by the next generation of gravitational wave detectors, we make an attempt to study the possible helicity coup
Externí odkaz:
https://doaj.org/article/4cd42fcd687c4b428b711ed12a99a55d
Publikováno v:
MNRAS, 415, 1093 (2011)
We investigate the dynamical effect of the turbulence in baryonic intergalactic medium (IGM) on the baryon fraction distribution. In the fully developed nonlinear regime, the IGM will evolve into the state of turbulence, containing strong and curved
Externí odkaz:
http://arxiv.org/abs/1103.1058
The dispersion measure(DM) of fast radio burst encodes important information such as its distance, properties of intervening medium. Based on simulations in the Illustris and IllustrisTNG projects, we analyze the DM of FRBs contributed by the interst
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::65154f726a2bcb63a6195feebf8bdc39
http://arxiv.org/abs/2210.14052
http://arxiv.org/abs/2210.14052
Supersonic motions are common in molecular clouds. (Sub)sonic turbulence is usually detected toward dense cores and filaments. However, it remains unknown whether (sub)sonic motions at larger scales ($\gtrsim$1~pc) can be present in different environ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::775dabbed8dbbb572bad1f3d111d5dd2
http://arxiv.org/abs/2203.14989
http://arxiv.org/abs/2203.14989
The spin of intergalactic filaments has been predicted from simulations, and supported by tentative evidence from redshift-space filament shapes in a galaxy redshift survey: generally, a filament is redshifted on one side of its axis, and blueshifted
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8941e517d991c71845c88f4868d35aa
The spatial distribution between dark matter and baryonic matter of the Universe is biased or deviates from each other. In this work, by comparing the results derived from IllustrisTNG and WIGEON simulations, we find that many results obtained from T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cbd83128bd560143ccb84aa035236efd
http://arxiv.org/abs/2111.05044
http://arxiv.org/abs/2111.05044
A large portion of the baryons at low redshifts are still missing from detection. Most of the missing baryons are believed to reside in large scale cosmic filaments. Understanding the distribution of baryons in filaments is crucial for the search for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::61d7bb98284035745fc26f03d3b7dc18
Quenching is a key topic in exploring the formation and evolution of galaxies. In this work, we study the quenching rate, i.e., the variation in the fraction of quenched galaxies per unit time, of the Illustris-1 simulation. By building the quenched
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2640e89899fac97d591fbbed899048a8
http://arxiv.org/abs/2011.09672
http://arxiv.org/abs/2011.09672