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ISBN10: 9027711100, ISBN13: 9789027711106, [publisher: D. Reidel Publishing Company] Softcover Volume 19. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. In poor condition, suitable as a reading copy. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,950grams, ISBN:9027711100 [Lincoln, United Kingdom] [Publication Year: 1980]
Date: 1980 Reidel paperback; light cover/corner wear; name on first end paper; pages clean/tight; good+ condition 1980. D. Reidel ISBN 9027711100 9789027711106 [US]
D. Reidel Publishing Company, Date: 1980. Volume 19. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. In poor condition, suitable as a reading copy. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,950grams, ISBN:9027711100 1980. D. Reidel Publishing Company ISBN 9027711100 9789027711106 [GB]
ISBN10: 9027711100, ISBN13: 9789027711106, [publisher: D. Reidel Publishing Company] Softcover Volume 19. This is an ex-library book and may have the usual library/used-book markings inside.This book has soft covers. In poor condition, suitable as a reading copy. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,950grams, ISBN:9027711100 [Lincoln, United Kingdom] [Publication Year: 1980]
Springer 1980 Paperback Fine Previous owner initials on front free page. Previous owner was Alexei Vladimir Filippenko (some books I have he has inked his name...some have just the initials as this one does)(1958-) is an American astrophysicist and professor of astronomy at the University of California, Berkeley. His research focuses on supernovae and active galaxies at optical, ultraviolet, and near-infrared wavelengths. Filippenko developed and runs the Katzman Automatic Imaging Telescope (KAIT), a fully robotic telescop.
ISBN10: 9027711100, ISBN13: 9789027711106, [publisher: Springer] Softcover Previous owner initials on front free page. Previous owner was Alexei Vladimir Filippenko (some books I have he has inked his name.some have just the initials as this one does)(1958-) is an American astrophysicist and professor of astronomy at the University of California, Berkeley. His research focuses on supernovae and active galaxies at optical, ultraviolet, and near-infrared wavelengths. Filippenko developed and runs the Katzman Automatic Imaging Telescope (KAIT), a fully robotic telescope which conducts the Lick Observatory Supernova Search (LOSS), the most successful nearby supernova search. He is also a member of the Nuker Team which uses the Hubble space telescope to examine supermassive black holes and determined the relationship between a galaxy's central black hole's mass and velocity dispersion. No other markings in book. Unread. [Novato, CA, U.S.A.] [Publication Year: 1980]
Springer, Date: 1980-11-30. Paperback. Like New. in x in x in. Previous owner initials on front free page. Previous owner was Alexei Vladimir Filippenko (some books I have he has inked his name...some have just the initials as this one does)(1958-) is an American astrophysicist and professor of astronomy at the University of California, Berkeley. His research focuses on supernovae and active galaxies at optical, ultraviolet, and near-infrared wavelengths. Filippenko developed and runs the Katzman Automatic Imaging Telescope (KAIT), a fully robotic telescope which conducts the Lick Observatory Supernova Search (LOSS), the most successful nearby supernova search. He is also a member of the Nuker Team which uses the Hubble space telescope to examine supermassive black holes and determined the relationship between a galaxy's central black hole's mass and velocity dispersion. No other markings in book. Unread. 1980. Springer ISBN 9027711100 9789027711106 [US]
D. Reidel Publishing Company 1980 Trade paperback Volume 19. This is an ex-library book and may have the usual library/used-book markings inside. This book has soft covers. In poor condition, suitable as a reading copy. Please note the Image in this listing is a stock photo and may not match the covers of the actual item, 950grams, ISBN: 9027711100.
ISBN10: 9027711100, ISBN13: 9789027711106, [publisher: Springer] Softcover No part of the Hertzsprung-Russell diagram shows a more pronounced diversity of stellar types than the upper part, which contains the most luminous stars. Can one visualize a larger difference than between a luminous, young and extremely hot Of star, and a cool, evolved pulsating giant of the Mira type, or an S-type supergiant, or - again at the other side of the diagram - the compact nucleus of a planetary nebula? But there is order and unity in this apparent disorder! Virtually all types of bright stars are evolutionally related, in one way or the other. Evolution links bright stars. In many cases the evolution is speeded up by, or at least intimately related to various signs of stellar instability. Bright stars lose mass, either continuously or in dramatic sudden events, they vibrate or pulsate - and with these tenuous, gigantic objects this often happens in a most bizarre fashion. Sometimes the evolution goes so fast that fundamental changes are observable in the time span of a human's life - several of such cases have now been identified. Softcover reprint of the original 1st ed. 1980. [Houston, TX, U.S.A.] [Publication Year: 1980]
ISBN10: 9027711100, ISBN13: 9789027711106, [publisher: Springer] Softcover All orders are dispatched the following working day from our UK warehouse. Established in 2004, we have over 500,000 books in stock. No quibble refund if not completely satisfied. [Llandybie, United Kingdom] [Publication Year: 1980]
Springer 1980 paperback Good All orders are dispatched within 1 working day from our UK warehouse. Established in 2004, we are dedicated to recycling unwanted books on behalf of a number of UK charities who benefit from added revenue through the sale of their books plus huge savings in waste disposal. No quibble refund if not completely satisfied.
ISBN10: 9027711100, ISBN13: 9789027711106, [publisher: Springer Netherlands] Softcover Druck auf Anfrage Neuware - Printed after ordering - No part of the Hertzsprung-Russell diagram shows a more pronounced diversity of stellar types than the upper part, which contains the most luminous stars. Can one visualize a larger difference than between a luminous, young and extremely hot Of star, and a cool, evolved pulsating giant of the Mira type, or an S-type supergiant, or - again at the other side of the diagram - the compact nucleus of a planetary nebula But there is order and unity in this apparent disorder! Virtually all types of bright stars are evolutionally related, in one way or the other. Evolution links bright stars. In many cases the evolution is speeded up by, or at least intimately related to various signs of stellar instability. Bright stars lose mass, either continuously or in dramatic sudden events, they vibrate or pulsate - and with these tenuous, gigantic objects this often happens in a most bizarre fashion. Sometimes the evolution goes so fast that fundamental changes are observable in the time span of a human's life - several of such cases have now been identified. [Einbeck, Germany] [Publication Year: 1980] ...
ISBN10: 9027711100, ISBN13: 9789027711106, [publisher: Springer Netherlands] Softcover Druck auf Anfrage Neuware - Printed after ordering - No part of the Hertzsprung-Russell diagram shows a more pronounced diversity of stellar types than the upper part, which contains the most luminous stars. Can one visualize a larger difference than between a luminous, young and extremely hot Of star, and a cool, evolved pulsating giant of the Mira type, or an S-type supergiant, or - again at the other side of the diagram - the compact nucleus of a planetary nebula But there is order and unity in this apparent disorder! Virtually all types of bright stars are evolutionally related, in one way or the other. Evolution links bright stars. In many cases the evolution is speeded up by, or at least intimately related to various signs of stellar instability. Bright stars lose mass, either continuously or in dramatic sudden events, they vibrate or pulsate - and with these tenuous, gigantic objects this often happens in a most bizarre fashion. Sometimes the evolution goes so fast that fundamental changes are observable in the time span of a human's life - several of such cases have now been identified. [Einbeck, Germany] [Publication Year: 1980] ...
Paperback / softback. New. No part of the Hertzsprung-Russell diagram shows a more pronounced diversity of stellar types than the upper part, which contains the most luminous stars. ISBN 9027711100 9789027711106 [GB]
ISBN10: 9027711100, ISBN13: 9789027711106, [publisher: Springer] Softcover Series: Geophysics and Astrophysics Monographs (Closed). Num Pages: 470 pages, biography. BIC Classification: PGS. Category: (P) Professional & Vocational. Dimension: 244 x 170 x 24. Weight in Grams: 870. . 1980. Softcover reprint of the original 1st ed. 1980. Paperback. . . . . Books ship from the US and Ireland. [Olney, MD, U.S.A.] [Publication Year: 1980]
ISBN10: 9027711100, ISBN13: 9789027711106, [publisher: Springer] Softcover Very Good [Redhill, SURRE, United Kingdom] [Publication Year: 1980]
DISCLOSURE:
When you click on links to various merchants on this site and make a purchase, this can result in this site earning a commission at no extra cost to you. Affiliate programs and affiliations include, but are not limited to, the eBay Partner Network, Amazon and Alibris.
