標(biāo)題: Titlebook: Astrophysics Is Easy!; An Introduction for Michael Inglis Book 2023Latest edition The Editor(s) (if applicable) and The Author(s), under e [打印本頁(yè)] 作者: obdurate 時(shí)間: 2025-3-21 17:12
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作者: opalescence 時(shí)間: 2025-3-21 23:28
The Hertzsprung-Russell Diagram,can now put all of these parameters together to form a picture of how a star evolves. This is often quite useful in many sciences to represent the characteristics, or data, about a group of objects in the form of a graph.作者: 熒光 時(shí)間: 2025-3-22 04:17 作者: 騷動(dòng) 時(shí)間: 2025-3-22 07:46 作者: 纖細(xì) 時(shí)間: 2025-3-22 11:23 作者: Abutment 時(shí)間: 2025-3-22 15:56 作者: APEX 時(shí)間: 2025-3-22 17:46
Setting Up the WPF Development Environment,can now put all of these parameters together to form a picture of how a star evolves. This is often quite useful in many sciences to represent the characteristics, or data, about a group of objects in the form of a graph.作者: terazosin 時(shí)間: 2025-3-22 23:57
Setting Up the WPF Development Environment,m to be any sort of material that lies between one star and another. At the same time, we know intuitively that this cannot be true, for if space were empty, from what did stars form? This then leads us to the conclusion that perhaps space is not quite so empty, but filled with some sort of material作者: 揭穿真相 時(shí)間: 2025-3-23 01:58
C#, XAML, and Object-Oriented Programming,r dies? After all, our planet is only 4.5 billion years old, and we have been studying astronomy for about the last 10,000?years. Well, fortunately for us, it is nevertheless possible to observe the many disparate ways in which a star can end its life.作者: CREEK 時(shí)間: 2025-3-23 08:43
https://doi.org/10.1007/978-1-4302-1951-4 be observed with a cosmological bias is limited. Nevertheless, there are a few that can be seen by an astute observer, and there is one seemingly simple question that can be asked that has profound consequences.作者: Root494 時(shí)間: 2025-3-23 11:45
https://doi.org/10.1007/978-3-031-16805-5Astronomical Observing Stars; Astrophysics Demystified; Astrophysics Explained; Astrophysics for Lay Re作者: nugatory 時(shí)間: 2025-3-23 15:41
978-3-031-16804-8The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerl作者: 匍匐前進(jìn) 時(shí)間: 2025-3-23 19:15 作者: muster 時(shí)間: 2025-3-24 00:00
Case Study D: SilverlightVideoPlayerProject,Before we discuss topics of astrophysics such as stars, black holes and galaxies, it is wise to begin our journey with our closest neighbours, namely the Solar System.作者: 廚房里面 時(shí)間: 2025-3-24 04:02 作者: paragon 時(shí)間: 2025-3-24 09:56 作者: 防銹 時(shí)間: 2025-3-24 12:13
C#, XAML, and Object-Oriented Programming,In this chapter, we shall look at the Sun, bearing in mind it is a star on the main sequence. With this approach, it is possible to use the Sun as a benchmark with which to compare stars of differing size.作者: 惰性女人 時(shí)間: 2025-3-24 15:34
https://doi.org/10.1007/978-1-4302-1951-4It may come as a surprise to know that nearly 50% of stars in the Milky Way are not single stars, but multiple stars, and many of these are . These, as we shall see, are very important in astrophysics as they allow us to determine the mass of stars, and the mass determines everything!作者: 夾克怕包裹 時(shí)間: 2025-3-24 20:48
Writing a Custom Content Panel,We have so far covered topics that describe how a star forms, how the mass of stars can be determined by observing binary-star systems, and how long it takes to become a star. Now we shall discuss how long a star will remain on the main sequence and then look at what happens due to changes in its internal structure.作者: 迅速飛過 時(shí)間: 2025-3-25 02:09
C#, XAML, and Object-Oriented Programming,We now turn our attention to high-mass stars. As you have probably surmised by now, the death throes of these stars are very different, and spectacular, compared with those of low-mass stars.作者: 擔(dān)憂 時(shí)間: 2025-3-25 04:10 作者: galley 時(shí)間: 2025-3-25 11:27 作者: AXIS 時(shí)間: 2025-3-25 14:16
https://doi.org/10.1007/978-1-4302-1951-4It is sobering to think that in a period of about 25?years our view of the universe has changed so much that we no longer believe that our Solar System is the only one but in fact is just one of many that exist in the Milky?Way.作者: Chagrin 時(shí)間: 2025-3-25 18:02
C#, XAML, and Object-Oriented Programming,Our galactic home is the Milky Way, but even though galaxies are faint ephemeral objects for must of us, they exist in many shapes, sizes and in numbers. Very big numbers - even an infinite amount of them作者: ENACT 時(shí)間: 2025-3-25 22:08
Writing a Custom Content Panel,We now discuss a type of galaxy that has become very prominent in astrophysical research over the past 20 or so years—. and ., or ..作者: mortuary 時(shí)間: 2025-3-26 02:32 作者: Exposition 時(shí)間: 2025-3-26 08:21 作者: 比喻好 時(shí)間: 2025-3-26 09:56 作者: Stagger 時(shí)間: 2025-3-26 13:26
Star Birth,Star birth is a process that involves a considerable number of astrophysical processes, yet can be explained fairly easily. This the is the subject of the chapter;?how, why and where?stars are born, and even why they differ from each other.作者: 臆斷 時(shí)間: 2025-3-26 16:49
Galactic Clusters and Stellar Associations,Look up at the night sky, and what do you see? Stars! In a telescope thousands, if not millions, will be seen. But surprisingly, the process of star birth, as we have seen, does not give rise to just one star over here, and another over there. Stars are formed in star clusters!作者: 卷發(fā) 時(shí)間: 2025-3-26 21:56
The Sun, Our Nearest Star,In this chapter, we shall look at the Sun, bearing in mind it is a star on the main sequence. With this approach, it is possible to use the Sun as a benchmark with which to compare stars of differing size.作者: Phenothiazines 時(shí)間: 2025-3-27 04:28 作者: 事物的方面 時(shí)間: 2025-3-27 08:08
Life on the Main Sequence,We have so far covered topics that describe how a star forms, how the mass of stars can be determined by observing binary-star systems, and how long it takes to become a star. Now we shall discuss how long a star will remain on the main sequence and then look at what happens due to changes in its internal structure.作者: 充足 時(shí)間: 2025-3-27 12:21
Star Death: Supernovae, & Neutron Stars,We now turn our attention to high-mass stars. As you have probably surmised by now, the death throes of these stars are very different, and spectacular, compared with those of low-mass stars.作者: 對(duì)待 時(shí)間: 2025-3-27 15:12 作者: 許可 時(shí)間: 2025-3-27 19:03 作者: Budget 時(shí)間: 2025-3-28 00:52 作者: 執(zhí)拗 時(shí)間: 2025-3-28 03:05
Galaxies,Our galactic home is the Milky Way, but even though galaxies are faint ephemeral objects for must of us, they exist in many shapes, sizes and in numbers. Very big numbers - even an infinite amount of them作者: AWL 時(shí)間: 2025-3-28 07:18
Active Galaxies,We now discuss a type of galaxy that has become very prominent in astrophysical research over the past 20 or so years—. and ., or ..作者: Awning 時(shí)間: 2025-3-28 14:04
The Speculative Universe,The final chapter deals with topics that are, at present, still highly hypothetical. As well as controversial. There is not enough observational or theoretical evidence to say with any certainty that these ideas are established, but rather, are hypotheses that may in the future be shown to be correct.作者: 浮雕寶石 時(shí)間: 2025-3-28 16:37 作者: CRP743 時(shí)間: 2025-3-28 21:02
Star Death: White Dwarfs and Planetary Nebulae,r dies? After all, our planet is only 4.5 billion years old, and we have been studying astronomy for about the last 10,000?years. Well, fortunately for us, it is nevertheless possible to observe the many disparate ways in which a star can end its life.作者: Dungeon 時(shí)間: 2025-3-29 02:21 作者: Mendicant 時(shí)間: 2025-3-29 04:31 作者: 歡騰 時(shí)間: 2025-3-29 09:56 作者: clarify 時(shí)間: 2025-3-29 12:34
C#, XAML, and Object-Oriented Programming,r dies? After all, our planet is only 4.5 billion years old, and we have been studying astronomy for about the last 10,000?years. Well, fortunately for us, it is nevertheless possible to observe the many disparate ways in which a star can end its life.作者: Legion 時(shí)間: 2025-3-29 18:58
https://doi.org/10.1007/978-1-4302-1951-4 be observed with a cosmological bias is limited. Nevertheless, there are a few that can be seen by an astute observer, and there is one seemingly simple question that can be asked that has profound consequences.作者: heartburn 時(shí)間: 2025-3-29 22:05
Michael InglisExplains the workings of the universe using nothing more than arithmetic and simple examples.Includes new material on gravitational waves, Special & General Relativity, exomoons, telescopes, black hol作者: 易于 時(shí)間: 2025-3-30 01:37
The Patrick Moore Practical Astronomy Serieshttp://image.papertrans.cn/b/image/163694.jpg作者: Terrace 時(shí)間: 2025-3-30 07:51 作者: 自制 時(shí)間: 2025-3-30 09:08 作者: 負(fù)擔(dān) 時(shí)間: 2025-3-30 14:12 作者: landmark 時(shí)間: 2025-3-30 20:18
Setting Up the WPF Development Environment, empty, from what did stars form? This then leads us to the conclusion that perhaps space is not quite so empty, but filled with some sort of material that, to our eyes, is all but invisible yet is responsible for providing the source material for stars.作者: 相一致 時(shí)間: 2025-3-30 22:24 作者: anticipate 時(shí)間: 2025-3-31 03:33 作者: CRACK 時(shí)間: 2025-3-31 06:39 作者: 察覺 時(shí)間: 2025-3-31 11:14 作者: interference 時(shí)間: 2025-3-31 14:08
A New Theory of T Truth Degree on , n-Valued Propositional Logic Systemthe concepts of t similarity degree, t pseudo-metric between propositional formulas, and t divergent degree and t consistent degree of theory . in . are obtained, and their correlation properties are discussed.作者: 信任 時(shí)間: 2025-3-31 18:54
Book 1998n access, for each specific problem, to its present status of solution as well as to the most up-to-date methods for approaching it. The main objective of the book is to explain some methods and new techniques, and to apply them. It deals with such important subjects as variational methods, the continuity method, parabolic equations on fiber.作者: Servile 時(shí)間: 2025-3-31 22:05 作者: Calculus 時(shí)間: 2025-4-1 04:28 作者: GRAIN 時(shí)間: 2025-4-1 10:01 作者: aspersion 時(shí)間: 2025-4-1 10:19 作者: Nmda-Receptor 時(shí)間: 2025-4-1 17:45 作者: 改變 時(shí)間: 2025-4-1 18:41 作者: fledged 時(shí)間: 2025-4-1 22:56
