ISM:molecules相关论文
To investigate the effects of massive star evolution on surrounding molecules,we select nine massive clumps previously o......
Quantifying the anisotropic density structure of the Central Molecular Zone-a 2D correlation functio
The Central Molecular Zone (CMZ) is a ring-like structure sitting at the center of the Milky Way.Using the 870 μtm cont......
Electron capture between solar wind ions and neutral species has contributed to the understanding of X-ray production fr......
Quantifying the anisotropic density structure of the Central Molecular Zone–a 2D correlation functio
The Central Molecular Zone(CMZ) is a ring-like structure sitting at the center of the Milky Way.Using the 870 μm contin......
To investigate the effects of massive star evolution on surrounding molecules,we select nine massive clumps previously o......
为探究吕家坨井田地质构造格局,根据钻孔勘探资料,采用分形理论和趋势面分析方法,研究了井田7......
We report here Atacama Large Millimeter/submillimeter Array (ALMA) N2H+ (1-0) images of the Orion Molecular Cloud 2 and ......
Laboratory study of the formation of fullerene(from smaller to larger,C44 to C70)/anthracene cluster
The formation and evolution mechanism of fullerenes in the planetary nebula or in the interstellar medium are still not ......
Astrochemical modeling is needed for understanding the formation and evolution of interstellar molecules,and for extract......
A filament is an important structure for studying star formation,especially intersections of filaments which are believe......
At low temperatures (～10 K),hydrogen atoms can diffuse quickly on grain ice mantles and frequently encounter hydrogen mol......
Thirty massive clumps associated with bright infrared sources were observed to detect the infall signatures and characte......
Stars form through the gravitational collapse of molecular cloud cores.Before collapsing,the cores are supported by ther......
In search of infall motion in molecular clumps Ⅱ:HCO+(1-0)and HCN(1-0)observations toward a sub-samp
Gravitational accretion accumulates the original mass.This process is crucial for us to understand the initial phases of......
Hydroxyacetone(CH3COCH2OH)is one of the smallest molecules that contain both hydroxyl and carbonyl group on neighboring ......
Data of 12CO/13CO/C18O J = 1 → 0 emission toward the Galactic plane region of l = 35°to 45° and b =-5° to +5° are a......
We present results of 13CO(1-0), C18O(1-O), and HCO+(1-0) map ob-servations and N2H+(1-O) single point observations dire......
We report here Atacama Large Millimeter/submillimeter Array(ALMA)N2H+(1-0)images of the Orion Molecular Cloud 2 and 3(OM......
Thirty massive clumps associated with bright infrared sources were observed to detect the infall signatures and characte......
Astrochemical modeling is needed for understanding the formation and evolution of interstellar molecules,and for extract......
Laboratory study of the formation of fullerene(from smaller to larger, C44 to C70)/anthracene cluste
The formation and evolution mechanism of fullerenes in the planetary nebula or in the interstellar medium are still not ......
The aim of the presented work is to analyze the impact of experimentally evaluated reactions of hydrogen abstraction on ......
That the laws of physics are the same at all times and places throughout the Universe is one of the basic assumptions of......
The gases of the interstellar medium(ISM) possess orders of magnitude more mass than those of all the stars combined and......
Theoretical approach to study the formation of C2H4O2 isomers in interstellar medium through reactio
The three isomers of C2H4O2,viz.,glycolaldehyde(HCOCH2 OH),acetic acid(CH3 COOH)and methyl formate(HCOOCH3),have been de......
The kinetic Monte Carlo simulation is a rigorous numerical approach to study the chemistry on dust grains in cold dense ......
