The subject is the mass of the three dominant, equilibrium cosmological objects: the irregular galaxy (dwarf), the regular galaxy (Hubble’s “tuning fork”), and the galactic cluster. The standard ΛCDM theory and a ...
This paper develops an original theory of dark matter in the current ΛCDM framework, whose main hypothesis is that DM is generated by the own gravitational field, according to an unknown quantum gravitational phenome...
support of the National Nature Science Foundation of China (Nos.12303017,and12203096);supported by Anhui Provincial Natural Science Foundation project No.2308085QA33;supported by the science research grants from the China Manned Space Project。
The large-scale imaging survey will produce massive photometric data in multi-bands for billions of galaxies.Defining strategies to quickly and efficiently extract useful physical information from this data is mandato...
supported by the National Natural Science Foundation of China(grant Nos.12422307,12373053,and 12321003);the Key Research Program of Frontier Sciences(grant No.ZDBS-LY-7014);Chinese Academy of Sciences,and the Natural Science Foundation of Jiangsu Province(grant No.BK20221562);supported by the Chinese Academy of Sciences President's International Fellowship Initiative(grant No.2023VMB0001)。
The[O iii]λλ4960,5008 emission lines in the optical spectra of galaxies and quasars have been widely used to investigate the possible variation of the fine-structure constantαover cosmic time.In this work,we utiliz...
partially supported by the National Natural Science Foundation of China (NSFC, grant Nos. 12433004, U2031201, and 11733001);Guangdong Major Project of Basic and Applied Basic Research (grant No. 2019B030302001);the science research grants from the China Manned Space Project with No. CMS-CSST-2021-A06;the support for Astrophysics Key Subjects of Guangdong Province and Guangzhou City;The Key Laboratory for Astronomical Observation and Technology of Guangzhou also supports the work。
A Very High-energy(VHE) flare was observed by Major Atmospheric Gamma Imaging Cherenkov Telescopes on MJD 57788. This VHE flare was characterized by increased VHE flux and short timescales. In this study, we used one-...
the National Natural Science Foundation of China(NSFC,Grant Nos.11921003,12233011,and 12373002)。
It was hypothesized in the literature that some physical parameters may be time-evolving and the astrophysical data can serve as a probe.Recently,the James Webb Space Telescope(JWST)released its early observations.In ...
financial support from the Secretaría Nacional de Ciencia,Tecnología e Innovación(SENACYT);the Departamento de Fortalecimiento a los Posgrados Nacionales and the coordination of the program“MOVILIDAD DE INVESTIGACIóN,”for the project“Formación de capacidades investigativas en la línea de Astronomía Extragaláctica 005-2023”;the support of the Programa de Apoyo a Proyectos de Investigación e Innovación Tecnológica(PAPIIT)IN108323 from the Dirección General de Asuntos del Personal Académico(DGAPA-UNAM)。
We analyzed the fractions of barred galaxies in the local Universe using a volume-limited sample of galaxies from the Sloan Digital Sky Survey Data Release 3.We examined 116 field galaxies with redshifts between 0.020...
supported by the National Key Research And Development Program of China(No.2022YFF0711500);the National Natural Science Foundation of China(NSFC,Grant No.12373097);the Basic and Applied Basic Research Foundation Project of Guangdong Province(No.2024A1515011503);the Guangzhou Science and Technology Funds(2023A03J0016)。
Open clusters(OCs)serve as invaluable tracers for investigating the properties and evolution of stars and galaxies.Despite recent advancements in machine learning clustering algorithms,accurately discerning such clust...
financial support from the National Natural Science Foundation of China(NSFC,No.12203028);supported by the research project of Qujing Normal University(2105098001/094);supported by the youth project of Yunnan Provincial Science and Technology Department(202101AU070146,2103010006);funding for the training Program for talents in Xingdian,Yunnan Province;supported by the NSFC(12121003,12192220,and 12192222);the science research grants from the China Manned Space Project with No.CMS-CSST-2021-A05;supported by the NSFC(11733001,U2031201 and 12433004)。
The theoretical model suggests that relativistic jets of active galactic nuclei(AGNs)rely on the black hole spin and/or accretion.We study the relationship between jet,accretion,and spin using supermassive black hole ...
One of the most important goals of modern cosmology is to understand how galaxies form and evolve in ecosystems defined by the cosmic density field. The formation of galaxies is a process through which cold baryonic g...