Environment Effects of the Stellar Mass Luminosity Function inside the Sixty Clusters of Galaxies at

来源 :2015年东亚青年天文学家会议 | 被引量 : 0次 | 上传用户:raulhanlin
下载到本地 , 更方便阅读
声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架
论文部分内容阅读
We conducting the investigation of the k-band selected stellar mass luminosity function inside the clusters,and the data sets we used are Sloan Digital Sky Survey (SDSS) DR10,and United Kingdom Infrared Digital Sky Survey (UKIDSS) of Large Area Survey (LAS) DR9.
其他文献
A combination of the available stratigraphical,structural and sedimentary information from NE Chinadefined a new tectonic process of NE Asian continental margin evolving from a continental block colli
In western Tibetan plateau,there are five sutures and four terranes between the Tarim block andHimalaya from north to south.Oytag-Kudi ophiolitic belt is the northernmost suture formed from the finalc
会议
近年来,时域瞬变场的这一装置和方法再次引起关注,并显示出了良好的应用前景.Alumbaugh(2002)提出采用近源瞬变电磁法对高阻目标体进行探测,Nestor(2009)认为近区探测具有可行性.Ziolkowski(2010)申报接地源近场瞬变电磁法发明专利.电性源瞬变电磁法的装备和软件开发得到越来越多的投入.对于深部目标探测来说,接地导线源瞬变电磁法可以在近场观测并获得较大的探测深度,比CSA
鄂尔多斯盆地西部主要包括西缘冲断带和天环向斜两大构造单元。西缘冲断带自南向北具有明显的分段特征,前人从不同角度得出了不尽相同的分段方案,但对造成分段的动力学机制涉及较少,研究也较薄弱。
The Planck satellite of ESA was launched 2009 from Kourou France Guyana.It measure temperature and polarization anisotropies of the cosmic microwave background radiation (CMB).
会议
In this work a 6.7GHz methanol maser targeting survey was made,using JVLA.In total,397 input sources are confirmed Class Ⅱ methanol masers chosen from the relative literatures.
会议
We present the spatially resolved kinematics of ionized gas and stars along the major axis of 9 pseudo bulge galaxies.
会议
Planetary small bodies are covered by a particle layer called regolith.The particle size and porosity of the regolith surface of small bodies are important physical properties.
会议
We present the search for sub-kilometer Trans-Neptunian Objects (TNOs) by re-examining the CoRoT (Convection Rotation and Planetary Transits) asteroseismology observations.
会议
The W51complex consist of couple of active star-formation regions.We intend to study the environment that surrounding those HII regions by means of radio recombination lines (RRLs).
会议