標(biāo)題: Titlebook: Galactic Radio Astronomy; Yoshiaki Sofue Book 2017 Springer Nature Singapore Pte Ltd. 2017 Galactic Astrophysics.Structure and Dynamics of [打印本頁(yè)] 作者: FLUX 時(shí)間: 2025-3-21 17:45
書目名稱Galactic Radio Astronomy影響因子(影響力)
書目名稱Galactic Radio Astronomy影響因子(影響力)學(xué)科排名
書目名稱Galactic Radio Astronomy網(wǎng)絡(luò)公開度
書目名稱Galactic Radio Astronomy網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Galactic Radio Astronomy被引頻次
書目名稱Galactic Radio Astronomy被引頻次學(xué)科排名
書目名稱Galactic Radio Astronomy年度引用
書目名稱Galactic Radio Astronomy年度引用學(xué)科排名
書目名稱Galactic Radio Astronomy讀者反饋
書目名稱Galactic Radio Astronomy讀者反饋學(xué)科排名
作者: limber 時(shí)間: 2025-3-21 20:32 作者: 較早 時(shí)間: 2025-3-22 00:46 作者: adj憂郁的 時(shí)間: 2025-3-22 05:35 作者: etiquette 時(shí)間: 2025-3-22 11:55 作者: cinder 時(shí)間: 2025-3-22 16:28 作者: cinder 時(shí)間: 2025-3-22 18:51 作者: 產(chǎn)生 時(shí)間: 2025-3-22 22:30
The Galactic Center and Activity, in general essentially the same. In this chapter various radio observational phenomena in the galactic center are reviewed and compared with those in active nuclei in galaxies. They are discussed in terms of energetic activities in the nuclear regions such as explosions and starbursts.作者: Compatriot 時(shí)間: 2025-3-23 02:02
Marc Castella,Eric Moreau,Vicente Zarzosoatter, which determine the dynamical properties of the galaxy. The IMS is deeply coupled to activities such as the star formation near the galactic plane, and is categorized as younger-generation matter in the galaxy, called Population I.作者: CHOKE 時(shí)間: 2025-3-23 06:21 作者: cluster 時(shí)間: 2025-3-23 12:02 作者: finale 時(shí)間: 2025-3-23 15:22
Advances in Human Clinical Nutritionetic field thus far observed reaches ～ 10. G on the surface of neutron stars observed as pulsars. Galactic magnetic fields are on the order of several 10. G or ～ 1 μG. Intergalactic fields are sometimes observed to exhibit about the same order as galactic, ～ 1 μG.The largest-scale, but weaker, magne作者: pester 時(shí)間: 2025-3-23 21:05 作者: Defense 時(shí)間: 2025-3-23 22:35
0075-8450 and black holes, galactic dynamics and dark-matter halos, magnetism of galaxies, interstellar gases in galaxies, and starbursts..A unique feature of this book is its focus on how to analyze and interpret radio978-981-10-3444-2978-981-10-3445-9Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: 色情 時(shí)間: 2025-3-24 05:13
Introduction,engths than the dust, and avoid scattering by dust particles. This situation mimics the reception of radio and TV waves even on a foggy and rainy day. If it is seen in radio, the radio galaxy appears quite different from its optical appearance..The change in appearance is not only because of the dif作者: Matrimony 時(shí)間: 2025-3-24 07:07 作者: rectum 時(shí)間: 2025-3-24 13:12
Advances in Hemostasis and Thrombosision Sagittarius. The interstellar matter (ISM) contains a significant amount of dust that hides most of the optical objects in the galactic disk from us. The optical absorption rate in the solar vicinity is about 1 mag per 1 kpc, and the galactic extinction amounts to ～ 30 mag for the light from the作者: 魅力 時(shí)間: 2025-3-24 16:51
Marc Castella,Eric Moreau,Vicente Zarzosoigh temperature (ionized gas, HII regions), high-energy particles (cosmic rays), and magnetic fields. They are embedded in the radiation field of stars. The ISM makes up approximately 10% of the mass of the galactic disk, and the majority is HI and H.. The remaining 90% is shared by stars and dark m作者: Loathe 時(shí)間: 2025-3-24 21:48 作者: Initial 時(shí)間: 2025-3-24 23:13
https://doi.org/10.1007/978-3-662-05613-4lack hole, a spheroidal central bulge composed of old stars, flat stellar disk filled with interstellar gas superposed by spiral arms, and a huge dark halo extending half-way to the neighboring galaxy..The galaxy is the nearest, hence most extensively observed galaxy in detail, however, the special 作者: Maximize 時(shí)間: 2025-3-25 06:57
Tobias K. Dallenga,Ulrich E. Schaibley useful object for understanding the nuclear activities of galaxies and their central black holes because of the small distance from us. Although nuclei of galaxies are not identical to the galactic center (GC), their fundamental physics and exhibited phenomena are in general similar, because the g作者: Cholesterol 時(shí)間: 2025-3-25 11:30 作者: headlong 時(shí)間: 2025-3-25 12:42
Yoshiaki SofueDescribes the interstellar physics and dynamics of the Galaxy and external galaxies with its consideration for students.Provides readers with knowledge of the underlying physics necessary to understan作者: scrape 時(shí)間: 2025-3-25 17:50 作者: pus840 時(shí)間: 2025-3-25 22:18 作者: 失眠癥 時(shí)間: 2025-3-26 00:19 作者: Anticoagulants 時(shí)間: 2025-3-26 08:19 作者: hidebound 時(shí)間: 2025-3-26 11:19
Interstellar Matter,igh temperature (ionized gas, HII regions), high-energy particles (cosmic rays), and magnetic fields. They are embedded in the radiation field of stars. The ISM makes up approximately 10% of the mass of the galactic disk, and the majority is HI and H.. The remaining 90% is shared by stars and dark m作者: 不確定 時(shí)間: 2025-3-26 15:38 作者: Asymptomatic 時(shí)間: 2025-3-26 18:45 作者: Priapism 時(shí)間: 2025-3-27 00:00 作者: Endemic 時(shí)間: 2025-3-27 01:16
Nonthermal Emission and Magnetic Fields,the galaxy. Analyses of polarization vectors and of Faraday rotation measures along the line of sight give us information about the three-dimensional orientation of magnetic fields.Magnetic fields are in pressure equilibrium with the interstellar medium on the order of ～ 10. ergs cm.. These fields a作者: Leisureliness 時(shí)間: 2025-3-27 05:59 作者: cushion 時(shí)間: 2025-3-27 10:17 作者: 宣誓書 時(shí)間: 2025-3-27 14:51
Reference work 2013Latest editioneld form the editorial board..The .Handbook of Combinatorial Optimization, second edition. is addressed to all scientists who use combinatorial optimization methods to model and solve problems. Experts in the field as well as non-specialists will find the material stimulating and useful..作者: Myocyte 時(shí)間: 2025-3-27 18:51 作者: Presbyopia 時(shí)間: 2025-3-27 22:06 作者: Capitulate 時(shí)間: 2025-3-28 05:50
Klaus North (.<. .) to random coil (.>. .)..Effect of calcium leads to an increase in ordering such that lipids are in their gel state up to 75 °C. Above this temperature a structural modification occurs which is not yet identified but which cannot be attributed to a conventional gel-to-fluid phase transition.作者: Ovulation 時(shí)間: 2025-3-28 10:17
A Biologically Inspired Approach to Collective Behaviors,onses on a scale larger than individuals themselves. Some of the examples around us include the coordinated movements of fish and birds in a school or a flock, respectively, the chemotactic aggregation of amoebae, the formation of lanes in densely packed human crowds, the generation of vortices in b作者: projectile 時(shí)間: 2025-3-28 11:26
G. Flattenbook is highly useful for graduate and postgraduate students on chemistry and its allied fields. It can also be used as a quick reference material byprofessionals working in the various fields of chemistry and material science..978-3-031-38357-1978-3-031-38355-7作者: GLOOM 時(shí)間: 2025-3-28 16:50
,L?sungen zu Verst?ndnisfragen und Aufgaben,uring the 2000s obscures the reality that, for large parts of the developing world, the challenges of development are more acute than ever. After three decades of Washington Consensus policies, deepening globalization, and China’s and India’s rapid growth and increasing international competitiveness
