论文部分内容阅读
Although hard to identify observationally,fly-by encounters between galaxies are believed to play an important role in galaxy evolution.
The Statistical Analysis of Interacting Dark Matter Halos
【摘 要】
：
Although hard to identify observationally,fly-by encounters between galaxies are believed to play an important role in galaxy evolution.
【机 构】
：
Yonsei University Korea Institute for Advanced St
【出 处】
：
2015年东亚青年天文学家会议
【发表日期】
：
2015年5期
其他文献
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
Environment Effects of the Stellar Mass Luminosity Function inside the Sixty Clusters of Galaxies at
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 Infrar
会议
The correlation between IR-to-UV luminosity ratio and UV color (or UV spectral slope),i.e.,the IRX-UV (or IRX-beta) relation,found in studies of starburst galaxies is a prevalent recipe for correcting
会议
Experimental study on propagation process of impact-induced seismic wave in quartz sand simulating a
Introduction:Recent spacecraft surveys clarify that the asteroid surface is covered with regolith made of boulders and pebbles such as that found on asteroid Itokawa by the Hayabusa spacecraft.
会议
We present the physical conditions of molecular hydrogen emission and their relation to dust and PAH emission towards some selected interstellar regions in the Large Magellanic Cloud.
会议
The evolved-star dust budget of the Small Magellanic Cloud from model fits to multi-epoch, multi-ban
Asymptotic giant branch (AGB) and red supergiant (RSG) stars dissipate their mass into the ISM in the form of slow winds over -10^(4-5) yr.
会议
PSR J2021 +4026 is the first variable gamma-ray pulsar detected by Fermi Large Area Telescope (LAT).Theres an unexpected decrease in flux of long-term light curves over a time scale shorter than a wee
会议
The COmpton Spectrometer and Imager (COSI),known as the Nuclear Compton Telescope (NCT) before,is a balloon-borne soft gamma-ray (0.2-5 MeV) telescope.
会议