An Introduction to the Sun and Stars
Cambridge University Press, Feb 26, 2004 - Science - 373 pages
Compiled by a team of experts, this textbook has been designed for elementary university courses in astronomy and astrophysics. Beginning with a discussion of our nearest star, the Sun, the volume then considers how astronomers study the basic physical properties and life-cycles of more distant stars. Exotic objects such as black holes are also introduced. The text contains numerous useful learning features such as boxed summaries, student exercises with full solutions, and a glossary of terms. It is also supported by a website hosting further teaching materials. Written in an accessible style that avoids complex mathematics, this book is suitable for self-study and will appeal to amateur astronomers as well as undergraduate students.
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THE WORKING SUN
THE FORMATION OF STARS
THE MAIN SEQUENCE LIFE OF STARS
THE LIFE OF STARS BEYOND THE MAIN
absorption lines accretion angular astronomers atoms axis binary system black hole brightness centre chromosphere convection core corona dense cloud disc distance Doppler dust Earth electromagnetic radiation electron elements emitted Equation flux density Galaxy gravitational H-R diagram helium burning hydrogen increase infrared interaction interstellar medium ionized line of sight luminosity magnetic field magnetic field lines main sequence main sequence lifetime main sequence stars mass number massive stars material measured molecules motion neutrinos neutron star nuclear reactions nuclei number density Observatory observed orbit parallax particles photon planetary nebula planets plasma ppl chain produce properties protostar pulsar QUESTION radio radius red giants region relative result rotation s-process Section shell shown in Figure shows solar activity solar wind spectral lines spectral type speed star's stellar evolution stellar wind Sun's sunspots supergiant surface telescope thermal typical variable visible light visual magnitude wavelength white dwarf X-ray y-rays