Titlebook: Cosmic Rays in Star-Forming Environments; Proceedings of the S Diego F. Torres,Olaf Reimer Conference proceedings 2013 Springer-Verlag Berl

Taft

書目名稱Cosmic Rays in Star-Forming Environments影響因子(影響力)




書目名稱Cosmic Rays in Star-Forming Environments影響因子(影響力)學(xué)科排名




書目名稱Cosmic Rays in Star-Forming Environments網(wǎng)絡(luò)公開度




書目名稱Cosmic Rays in Star-Forming Environments網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Cosmic Rays in Star-Forming Environments被引頻次




書目名稱Cosmic Rays in Star-Forming Environments被引頻次學(xué)科排名




書目名稱Cosmic Rays in Star-Forming Environments年度引用




書目名稱Cosmic Rays in Star-Forming Environments年度引用學(xué)科排名




書目名稱Cosmic Rays in Star-Forming Environments讀者反饋




書目名稱Cosmic Rays in Star-Forming Environments讀者反饋學(xué)科排名

擁擠前

Martina Zeleňáková,Abdelazim M. Negmexternal galaxies. We will review the methodologies employed to determine the cosmic ray ionization rates in the ISM, how cosmic rays rates can influence the determination of the mass of a galaxy and, finally, how cosmic rays affect star formation and its rate.

畏縮

Explosive

BIBLE

D. Káposztásová,Z. Vranayová,P. Purczl stellar radiation propagating through the dusty ISM of galaxies. It is in such CR-dominated regions (CRDRs) rather than Photon-dominated regions (PDRs) of H. clouds where the star formation initial conditions are set, making CRs the ultimate star-formation feedback factor in galaxies, able to oper

Expediency

How to Reach a Point of No Return,o determine the cosmic-ray ionisation rate (especially the cosmic-ray spectrum at . < 1 GeV and the ionisation cross sections), and calculate the ionisation rate as a function of the column density of molecular hydrogen. Available data support the existence of a low-energy component (below ～ 100 MeV

Expediency

CHOIR

澄清

pulmonary-edema

Space as the Next Theater of War,. These processes drive the chemical pathways of formation of gas phase molecules which later can be adsorbed onto the surface of grains. We improve on previously existing chemical models by treating the interaction of cosmic rays with the gas/grain environment in a way that is consistent with the l