“China-Chile Proposal”的版本间差异
跳到导航
跳到搜索
（Created page with "'''China-Chile Joint Research Fund 2016''' ==Project presentation== *Title: :Star Formation History of Galaxies in Different Environments from MaNGA Spectra *Abstract (<100..."） |
|||
| 第3行： | 第3行： | ||
==Project presentation== |
==Project presentation== |
||
| ⚫ | |||
*Title: |
|||
| ⚫ | |||
*Abstract (<1000 words): |
*Abstract (<1000 words): |
||
In the present–day galaxy population, it is well known that there is a strong relation between the properties of galaxies and their stellar masses and environments (Peng et al., 2010, 2012). However, the relative importance of secular evolution (nature) over nurture is not yet clear. Separating the effects of interaction–driven evolution in the observed galaxy properties is not trivial. |
In the present–day galaxy population, it is well known that there is a strong relation between the properties of galaxies and their stellar masses and environments (Peng et al., 2010, 2012). However, the relative importance of secular evolution (nature) over nurture is not yet clear. Separating the effects of interaction–driven evolution in the observed galaxy properties is not trivial. |
||
:- MaNGA spectra and galaxy properties |
|||
:- SED modelling |
|||
:- Experience of the team working with MaNGA data |
|||
:- Experience of the team working together and how this research funding would help in the development of the projects |
|||
:- Implementation and involvement of Chile researches on MaNGA |
|||
2016年10月13日 (四) 00:49的版本
China-Chile Joint Research Fund 2016
Project presentation
- Title: :Star Formation History of Galaxies in Different Environments from MaNGA Spectra
- Abstract (<1000 words):
In the present–day galaxy population, it is well known that there is a strong relation between the properties of galaxies and their stellar masses and environments (Peng et al., 2010, 2012). However, the relative importance of secular evolution (nature) over nurture is not yet clear. Separating the effects of interaction–driven evolution in the observed galaxy properties is not trivial.
- - MaNGA spectra and galaxy properties
- - SED modelling
- - Experience of the team working with MaNGA data
- - Experience of the team working together and how this research funding would help in the development of the projects
- - Implementation and involvement of Chile researches on MaNGA