標題: Titlebook: Extragalactic Astronomy and Cosmology; An Introduction Peter Schneider Textbook 20061st edition Springer-Verlag Berlin Heidelberg 2006 Cosm [打印本頁] 作者: Helmet 時間: 2025-3-21 18:22
書目名稱Extragalactic Astronomy and Cosmology影響因子(影響力)
書目名稱Extragalactic Astronomy and Cosmology影響因子(影響力)學(xué)科排名
書目名稱Extragalactic Astronomy and Cosmology網(wǎng)絡(luò)公開度
書目名稱Extragalactic Astronomy and Cosmology網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Extragalactic Astronomy and Cosmology被引頻次
書目名稱Extragalactic Astronomy and Cosmology被引頻次學(xué)科排名
書目名稱Extragalactic Astronomy and Cosmology年度引用
書目名稱Extragalactic Astronomy and Cosmology年度引用學(xué)科排名
書目名稱Extragalactic Astronomy and Cosmology讀者反饋
書目名稱Extragalactic Astronomy and Cosmology讀者反饋學(xué)科排名
作者: 不可比擬 時間: 2025-3-21 23:59 作者: HUMP 時間: 2025-3-22 01:31 作者: 違抗 時間: 2025-3-22 06:11 作者: 圓木可阻礙 時間: 2025-3-22 11:07
Informationsintegration in Biodatenbankenearly 8000 objects, most of them galaxies. In 1912, Vesto Slipher found that the spiral nebulae are rotating, using spectroscopic analysis. But the nature of these extended sources, then called nebulae, was still unknown at that time; it was unclear whether they are part of our Milky Way or outside it.作者: garrulous 時間: 2025-3-22 16:19 作者: garrulous 時間: 2025-3-22 18:08
The World of Galaxies,early 8000 objects, most of them galaxies. In 1912, Vesto Slipher found that the spiral nebulae are rotating, using spectroscopic analysis. But the nature of these extended sources, then called nebulae, was still unknown at that time; it was unclear whether they are part of our Milky Way or outside it.作者: 古老 時間: 2025-3-23 01:02
tic astronomy and proven textbook author.Fills a need for a .Starting with the description of our home galaxy the Milky Way, this cogently written textbook introduces the reader to the astronomy of galaxies, their structure, active galactic nuclei, evolution and large scale distribution. Then, from 作者: 錢財 時間: 2025-3-23 05:16 作者: fulmination 時間: 2025-3-23 08:01
Cosmology I: Homogeneous Isotropic World Models,e Universe is homogeneous when averaged over large spatial scales. Aspects of inhomogeneous cosmology, and thus the formation and evolution of structures in the Universe, will be considered later in Chap. 7.作者: GRIN 時間: 2025-3-23 13:23 作者: 培養(yǎng) 時間: 2025-3-23 17:31 作者: Fermentation 時間: 2025-3-23 21:50
https://doi.org/10.1007/978-3-642-59264-5ich we are able to study astrophysical processes in detail. Therefore, our journey through extragalactic astronomy will begin in our home Galaxy, with which we first need to become familiar before we are ready to take off into the depths of the Universe. Knowing the properties of the Milky Way is indispensable for understanding other galaxies.作者: rheumatology 時間: 2025-3-24 02:02
Vorgehensweise der empirischen Untersuchung,he projection of bright galaxies on the sky (see Figs. 6.1 and 6.2). The Milky Way itself is a member of a group, called the Local Group (Sect. 6.1), which implies that we are living in a locally overdense region of the Universe.作者: Ballad 時間: 2025-3-24 05:23
Information als Wettbewerbsfaktor,ption of a (spatially) homogeneous and isotropic Universe. Of course, the assumption of homogeneity is justified only on large scales because observations show us that our Universe is inhomogeneous on small scales – otherwise no galaxies or stars would exist.作者: cauda-equina 時間: 2025-3-24 07:37
The Milky Way as a Galaxy,ich we are able to study astrophysical processes in detail. Therefore, our journey through extragalactic astronomy will begin in our home Galaxy, with which we first need to become familiar before we are ready to take off into the depths of the Universe. Knowing the properties of the Milky Way is indispensable for understanding other galaxies.作者: octogenarian 時間: 2025-3-24 13:13 作者: cortex 時間: 2025-3-24 18:20 作者: HARD 時間: 2025-3-24 22:53 作者: 裝入膠囊 時間: 2025-3-25 02:07 作者: 樂器演奏者 時間: 2025-3-25 06:50
https://doi.org/10.1007/978-3-642-59264-5ich we are able to study astrophysical processes in detail. Therefore, our journey through extragalactic astronomy will begin in our home Galaxy, with which we first need to become familiar before we are ready to take off into the depths of the Universe. Knowing the properties of the Milky Way is in作者: 焦慮 時間: 2025-3-25 09:49 作者: 宣傳 時間: 2025-3-25 13:36
,überbetriebliche Informationsintegration,instead we will turn our attention to the space and time in which these objects are embedded. These considerations will then lead to a world model, the model of our cosmos. .This chapter will deal with aspects of homogeneous cosmology. As we will see, the Universe can, to first approximation, be con作者: 大笑 時間: 2025-3-25 17:46
Von der “Arriflex” zum “Fly-away”is is thermal radiation since the emitting plasma in stellar atmospheres is basically in thermodynamical equilibrium. To a first approximation, the spectral properties of a star can be described by a Planck spectrum whose temperature depends on the stellar mass and the evolutionary state of the star作者: insincerity 時間: 2025-3-25 21:17
Vorgehensweise der empirischen Untersuchung,he projection of bright galaxies on the sky (see Figs. 6.1 and 6.2). The Milky Way itself is a member of a group, called the Local Group (Sect. 6.1), which implies that we are living in a locally overdense region of the Universe.作者: compel 時間: 2025-3-26 03:49
Information als Wettbewerbsfaktor,ption of a (spatially) homogeneous and isotropic Universe. Of course, the assumption of homogeneity is justified only on large scales because observations show us that our Universe is inhomogeneous on small scales – otherwise no galaxies or stars would exist.作者: Adornment 時間: 2025-3-26 07:11
,Elektronische Marktpl?tze und Beschaffung,ies, and AGNs that we have gained in the other chapters, we are now ready to discuss the determination of the various cosmological parameters. In the course of this discussion, we will describe a number of methods, each of which is in itself useful for estimating cosmological parameters, and we will作者: 喪失 時間: 2025-3-26 09:00 作者: 歡樂中國 時間: 2025-3-26 14:47 作者: Aboveboard 時間: 2025-3-26 18:06
Informationsmanagement im MittelstandIn the final chapter of this book, we will dare to give an outlook for the fields of extragalactic astronomy and cosmology for the next few years from the perspective of 2006.作者: Abjure 時間: 2025-3-26 22:46 作者: 檔案 時間: 2025-3-27 03:47
Introduction and Overview,ge representative of the class of spiral galaxies. Two other examples of spiral galaxies are shown in Fig. 1.1 and Fig. 1.2, one of which we are viewing from above (face-on), the other from the side (edge-on). These are all stellar systems in which the majority of stars are confined to a relatively 作者: 真實的你 時間: 2025-3-27 08:10 作者: Jogging 時間: 2025-3-27 10:32 作者: tenuous 時間: 2025-3-27 15:25
Cosmology I: Homogeneous Isotropic World Models,instead we will turn our attention to the space and time in which these objects are embedded. These considerations will then lead to a world model, the model of our cosmos. .This chapter will deal with aspects of homogeneous cosmology. As we will see, the Universe can, to first approximation, be con作者: 人類 時間: 2025-3-27 18:22 作者: Extort 時間: 2025-3-27 23:30
Clusters and Groups of Galaxies,he projection of bright galaxies on the sky (see Figs. 6.1 and 6.2). The Milky Way itself is a member of a group, called the Local Group (Sect. 6.1), which implies that we are living in a locally overdense region of the Universe.作者: PANEL 時間: 2025-3-28 03:24
Cosmology II: Inhomogeneities in the Universe,ption of a (spatially) homogeneous and isotropic Universe. Of course, the assumption of homogeneity is justified only on large scales because observations show us that our Universe is inhomogeneous on small scales – otherwise no galaxies or stars would exist.作者: 燒瓶 時間: 2025-3-28 06:21 作者: Hyperlipidemia 時間: 2025-3-28 10:27
The Universe at High Redshift, This might have given the impression that, with the determination of the values for ., ., etc., cosmology is nearing its conclusion. As a matter of fact, for several decades cosmologists have considered the determination of the density parameter and the expansion rate of the Universe their prime ta作者: 使熄滅 時間: 2025-3-28 16:34
Textbook 20061st editiont admiration for the workings of the universe that shines through the lines and the many supporting color illustrations will deeply inspire the reader...While this book has grown out of introductory university courses on astronomy and astrophysics, it will not only be appreciated by undergraduate st作者: 波動 時間: 2025-3-28 20:25
upporting color illustrations will deeply inspire the reader...While this book has grown out of introductory university courses on astronomy and astrophysics, it will not only be appreciated by undergraduate st978-3-642-06971-0978-3-540-33175-9作者: nauseate 時間: 2025-3-29 02:15 作者: abstemious 時間: 2025-3-29 07:04
Nutzung webbasierter Plattformen,primitive initial state into what we are observing around us today – galaxies of different morphologies, the largescale structure of their distribution, clusters of galaxies, and active galaxies. We seek to study the formation of stars and ofmetals, and also the processes that reionized the intergal作者: 贊成你 時間: 2025-3-29 09:15
Active Galactic Nuclei,k spectra from a temperature range that covers about one decade. Since the Planck spectrum has a very narrow energy distribution around its maximum at h Pν ～ 3k BT, the spectrum of a galaxy is basically confined to a range between ～ 4000 ? and ～ 20 000 ?. If the galaxy is actively forming stars, you作者: entitle 時間: 2025-3-29 13:21 作者: LITHE 時間: 2025-3-29 19:03
- und Leistungsrechnung aktiv wiederholt und geübt werden. Das Aufgabenangebot kann direkt im Buch bearbeitet und mit ausführlich dargestellten L?sungen verglichen werden. Dies erm?glicht – unterstützt durch Exkurse und Cognitive-Maps – einen nachhaltigen Lernerfolg.978-3-8349-6316-1作者: BLINK 時間: 2025-3-29 22:08
,Zusammenfassung und Ausblick – eine Vision,mmel bekannt. Assyrien und Babylon waren frühe Zentren des Gewürzhandels. Vor Jahrtausenden benutzte man würzende Zutaten bereits in Indien und China. Schlie?lich sch?tzte man bereits lange vor Kolumbus’ Reisen die Vorzüge der Gewürze auch in Amerika.
