Titlebook: Astrophysics Is Easy!; An Introduction for Michael Inglis Book 2023Latest edition The Editor(s) (if applicable) and The Author(s), under e

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https://doi.org/10.1007/978-3-031-16805-5Astronomical Observing Stars; Astrophysics Demystified; Astrophysics Explained; Astrophysics for Lay Re

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978-3-031-16804-8The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerl

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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.

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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.

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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!

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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.

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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.