Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Ruixiang Chang"'
Publikováno v:
The Astrophysical Journal, Vol 976, Iss 1, p 15 (2024)
Narrow emission lines in a galaxy’s spectrum that show double peaks indicate the presence of distinct gas components with different velocities, and its physical origin remains uncertain. This study uses galaxies from the final MaNGA data release to
Externí odkaz:
https://doaj.org/article/8ab7cd3ba4e54379a76a72e233a4a56e
Autor:
María del Carmen Argudo Fernández, Fangting Yuan, Shiyin Shen, Jun Yin, Ruixiang Chang, Shuai Feng
Publikováno v:
Galaxies, Vol 3, Iss 4, Pp 156-163 (2015)
We present preliminary results of the spectral analysis on the radial distributions of the star formation history in both a galaxy merger and a spiral isolated galaxy observed with MaNGA. We find that the central part of the isolated galaxy is compos
Externí odkaz:
https://doaj.org/article/d0e0343344f54907a977fbc5596b40ac
Autor:
Jun Yin, Shiyin Shen, Ruixiang Chang, Lei Hao, Fang-Ting Yuan, Maria Argudo-Fernández, Médéric Boquien
Publikováno v:
Proceedings of the International Astronomical Union. 15:60-64
The star formation history (SFH) of galaxies allow us to investigate when galaxies formed their stars and assembled their mass. We can constrain the SFH with high level of precision from galaxies with resolved stellar populations, since we are able t
An analytical chemical evolution model is constructed to investigate the radial distribution of gas-phase and stellar metallicity for star-forming galaxies. By means of the model, the gas-phase and stellar metallicity can be obtained from the stellar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1547944cc81b758b4684777dd48d96f5
Publikováno v:
Proceedings of the International Astronomical Union. 14:271-273
Understanding the effect of environment on galaxy formation and evolution is one of the hot topics in extragalactic astronomy. Here we constructed a chemical evolution model of disk galaxies. By comparing the model predictions with the observed profi
Autor:
Yaqian Wu, Jing Li, Yan Xu, Gang Zhao, Chao Liu, Lan Zhang, Jing Zhong, Jeffrey L. Carlin, Bo Zhang, Hao Tian, Chengqun Yang, Rene A. Mendez, Xiang-Xiang Xue, Hans-Walter Rix, Ruixiang Chang
Publikováno v:
The Astrophysical Journal. 910:46
We characterize the kinematic and chemical properties of 589 Galactic Anticenter Substructure Stars (GASS) with K-/M- giants in Integrals-of-Motion space. These stars likely include members of previously identified substructures such as Monoceros, A1
NGC\,2403, NGC\,300 and M33 are three nearby pure-disc galaxies with similar stellar mass in different environments, they are benchmarks for understanding late-type spiral galaxies in different environments. The chemical evolution and growth of their
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24352f506e7b400e940e2f7a65ee5edc
http://arxiv.org/abs/1704.07697
http://arxiv.org/abs/1704.07697
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 426:1455-1464
We construct a parameterized model to explore the main properties of the star formation history of M33. We assume that the disk originates and grows by the primordial gas infall and adopt the simple form of gas accretion rate with one free parameter,
Publikováno v:
Dyes and Pigments. 88:307-314
A series of N -heteroaryl-1,8-naphthalimides with good sensitivity to solvent polarity were prepared. Empirical and quantum calculations showed that the electron withdrawing effect of the heteroaryl group increases the change in dipole moment on exci
Publikováno v:
The Astrophysical Journal. 705:1496-1502
The Tully-Fisher relation of spiral galaxies shows notable dependence on morphological types, with earlier type spirals having systematically lower luminosity at fixed maximum rotation velocity $V_{max}$. This decrement of luminosity is more signific