Philanthropist
发表于 2025-3-21 16:56:52
书目名称Environment and the Formation of Galaxies: 30 years later影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0312476<br><br> <br><br>书目名称Environment and the Formation of Galaxies: 30 years later影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0312476<br><br> <br><br>书目名称Environment and the Formation of Galaxies: 30 years later网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0312476<br><br> <br><br>书目名称Environment and the Formation of Galaxies: 30 years later网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0312476<br><br> <br><br>书目名称Environment and the Formation of Galaxies: 30 years later被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0312476<br><br> <br><br>书目名称Environment and the Formation of Galaxies: 30 years later被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0312476<br><br> <br><br>书目名称Environment and the Formation of Galaxies: 30 years later年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0312476<br><br> <br><br>书目名称Environment and the Formation of Galaxies: 30 years later年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0312476<br><br> <br><br>书目名称Environment and the Formation of Galaxies: 30 years later读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0312476<br><br> <br><br>书目名称Environment and the Formation of Galaxies: 30 years later读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0312476<br><br> <br><br>
jeopardize
发表于 2025-3-21 23:28:45
The Cosmic Mass Density Field Reconstruction from the SDSS Group Catalog,roduced by . The method uses the mass distribution in and around dark matter structures computed from cosmological simulations to map the cosmic mass distribution. This approach enables us to make reconstructions of the density field avoiding the use of arbitrary
Carcinoma
发表于 2025-3-22 02:18:25
The Void Galaxy Survey,entified voids in the SDSS redshift survey on the basis of a unique geometric technique, with no a prior selection of intrinsic properties of the void galaxies. The project intends to study in detail the gas content, star formation history and stellar content, as well as kinematics and dynamics of v
Malfunction
发表于 2025-3-22 08:38:41
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engrave
发表于 2025-3-22 08:47:59
The Dependence of Low Redshift Galaxy Properties on Environment,, group-centric radius, and the distinction between centrals and satellites; examined galaxy properties include star formation rate, colour, AGN fraction, age, metallicity and concentration. In general, satellite galaxies diverge more markedly from their central counterparts if they reside in more m
AVOID
发表于 2025-3-22 15:44:51
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AVOID
发表于 2025-3-22 20:07:27
The Fossil Candidate RX J1548.9+0851,ynamical friction as the driving process leads to the coalescence of individual galaxies in ordinary poor groups, leaving behind nothing more than a central, massive elliptical galaxy supposed to contain the merger history of the whole group. Due to longer merging timescales for less-massive galaxie
GROSS
发表于 2025-3-23 00:30:43
The Environments of Luminous Infrared Galaxies,arks an important luminosity point among IR galaxies - the large scale density of environment around LIRGs correlates strongly with their SFR above this value at a fixed stellar mass. On the other hand there is no clear correlation between stellar mass and density at constant SFR. No matter what the
智力高
发表于 2025-3-23 01:26:50
,UV–IR Luminosity Functions and Stellar Mass Functions of Galaxies in the Shapley Supercluster Core, z = 0.048, in order to investigate how the dense environment affects the galaxy properties, such as star formation (SF) or stellar mass. We find that, while the faint-end slope of optical and NIR LFs steepens with decreasing density, no environment effect is found in the slope of the SMFs. This su
增减字母法
发表于 2025-3-23 09:22:29
Component Luminosity Functions of Galaxy Pairs in the MGC,ging systems (Casteels and Patton 2011). Using mock catalogues, the effect of imposing a fixed magnitude separation (.) between galaxy pairs (to isolate major mergers) is explored and we find that imposing a . introduces a selection bias which must be corrected for when comparing with field LFs. Our