Roman Sorochenko (35 results)
Language: English
Published by Kluwer, 1990
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
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Condition: Very Good. 298 pp., hardcover, previous owner's name to front free endpaper else very good. - If you are reading this, this item is actually (physically) in our stock and ready for shipment once ordered. We are not bookjackers. Buyer is responsible for any additional duties, taxes, or fees required by recipient's coun…try.
Language: English
Published by Springer, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
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Language: English
Published by Kluwer, 1990
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
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Language: English
Published by Springer, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
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Language: English
Published by Springer 2013-10-04, 2013
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
- Softcover
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Language: English
Published by Springer, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
- Softcover
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Condition: New. pp. 316.
Language: English
Published by Springer, 2013
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
- Softcover
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Paperback. Condition: Brand New. 316 pages. 9.25x6.10x0.75 inches. In Stock.
More imagesLanguage: English
Published by Springer, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
- Softcover
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Taschenbuch. Condition: Neu. Radio Recombination Lines: 25 Years of Investigation | Proceeding of the 125th Colloquium of the International Astronomical Union, Held in Puschino, U.S.S.R., September 11-16, 1989 | M. A. Gordon (u. a.) | Taschenbuch | Astrophysics and Space Science Library | 312 S. | Englisch | 2011 | Springer | EA…N 9789401067683 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.
Language: English
Published by Springer Netherlands, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
- Softcover
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Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - Text no 1 Radio Recombination Lines (RRLs), discovered in the USSR in 1964, have become a powerful research tool for astronomers. Available throughout the radio spectrum, these lines carry information regarding the density, temperature, turbulence…and velocity of thermal plasmas. Their very existance shows the presence of thermal gas. They also can carry information regarding magnetic fields if Zeeman splitting were to be detected. Containing the proceedings of an IAU Colloquium celebrating the 25th anniversary of their detection, this volume tells us what has happened since. It contains the story of the detection of RRLs and reviews of many areas of physics of the interstellargas from which stars form, HII regions excited by newly formed stars, planetary nebulae involving dying stars, and the structure of our Milky Way and other galaxies reflecting the large-scale morphology of the star formation process. In addition there is an article describing modern laboratory studies of Rydberg atoms to probe the basic physics of atomic structure, and articles describing the theory of collisions and radiation upon Rydberg atoms leading to observate effects to be used as diagnostic tools in astromony. This book focuses on the 25 years of astronomical research with radio recombination lines (RRLs) since their discovery in 1965. It covers a wide range of topics: papers dealing with research into Rydberg atoms both in the laboratory and in the interstellar medium of our galaxy and others; papers on the interaction of radiation and atomic systems, as well as with the effects of inadiabatic collisions between these atoms and both ions and electrons. It deals with astronomical observations of atoms with `diameters' ranging from 0.08 to 50 mum a size factor of 625. It deals with RRLs in absorption, in emission and as true masers. And it deals with plasmas with temperatures ranging from 10 to greater than 104 kelvins, andwith an even greater range of volume densities. Much new work is reported, including low frequency RRLs discovered in 1980 and the maser RRLs from the star MWC349, discovered in 1989. The advent of aperture synthesis telescopes and large single-element telescopes have made possible RRL studies with high angular resolution. The sum total of the work reported here will make the volume a platform from which to search new horizons in RRL research.
Language: English
Published by Springer, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
- Softcover
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Language: English
Published by Springer, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
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Language: English
Published by Springer, 2002
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
- Hardcover
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Condition: New. In.
Language: English
Published by Springer, 2012
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
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Language: English
Published by Springer, 2012
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
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Language: English
Published by Springer Netherlands, 2012
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
- Softcover
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Language: English
Published by Springer Netherlands, 2002
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
- Hardcover
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Language: English
Published by Springer, 2012
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
- Softcover
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Condition: New. pp. xvii + 358 Indexes.
Language: English
Published by Springer, 2002
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
- Hardcover
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Condition: New. pp. 380 Indexes.
Language: English
Published by Springer Netherlands, Springer Netherlands, 2002
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
- Hardcover
Seller: AHA-BUCH GmbH, Einbeck, GermanyAHA-BUCH GmbH
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Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - Recombination lines at radio wavelengths have been - and still are - a pow erful tool for modern astronomy. For more than thirty years they have allowed astronomers to probe the gases from which stars form. They have even been detected in the Sun. In addi…tion, observations of these spectral lines facilitate basic research into the atom, in forms and environments that can only exist in the huge dimensions and extreme conditions of cosmic laboratories. We intend this book to serve as a tourist's guide to the world of Radio Recombination Lines. It contains three divisions: a history of their discovery, the physics of how they form and how their voyage to us influences their spectral profiles, and a description of their many astronomical contributions to date. The appendix includes supplementary calculations that may be useful to some astronomers. This material also includes tables of line frequencies from 12 MHz to 30THz (AlOJLm) as well as FORTRAN computer code to calculate the fine structure components of the lines, to evaluate radial matrix integrals, and to calculate the departure coefficients of hydrogen in a cosmic environment. It also describes how to convert observational to astrophysical units. The text includes extensive references to the literature to assist readers who want more details.
Language: English
Published by Springer Netherlands, Springer, 2012
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
- Softcover
Seller: AHA-BUCH GmbH, Einbeck, GermanyAHA-BUCH GmbH
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Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - Recombination lines at radio wavelengths have been - and still are - a pow erful tool for modern astronomy. For more than thirty years they have allowed astronomers to probe the gases from which stars form. They have even been detected in the Sun.…In addition, observations of these spectral lines facilitate basic research into the atom, in forms and environments that can only exist in the huge dimensions and extreme conditions of cosmic laboratories. We intend this book to serve as a tourist's guide to the world of Radio Recombination Lines. It contains three divisions: a history of their discovery, the physics of how they form and how their voyage to us influences their spectral profiles, and a description of their many astronomical contributions to date. The appendix includes supplementary calculations that may be useful to some astronomers. This material also includes tables of line frequencies from 12 MHz to 30THz (AlOJLm) as well as FORTRAN computer code to calculate the fine structure components of the lines, to evaluate radial matrix integrals, and to calculate the departure coefficients of hydrogen in a cosmic environment. It also describes how to convert observational to astrophysical units. The text includes extensive references to the literature to assist readers who want more details.
Language: English
Published by Springer, 2012
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
- Softcover
Seller: Mispah books, Redhill, SURRE, United KingdomMispah books
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Language: English
Published by Springer, 2012
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
- Softcover
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Condition: As New. Unread book in perfect condition.
Published by Moscow, 1975
- Hardcover
Seller: BiblioEra, Everett, MA, U.S.A.BiblioEra
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Hardcover. Condition: Good. In Russian. Sorochenko, Roman Leonidovich. Report on mission to Germany. Moscow: 1975. All images are for identification of editions only. Several books of the same edition may be available. Please feel free to request photos of available books.SKU7001864.
Language: English
Published by Springer, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
- Softcover
- Print on Demand
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Language: English
Published by Springer, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
- Softcover
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Condition: New. Print on Demand pp. 316 49:B&W 6.14 x 9.21 in or 234 x 156 mm (Royal 8vo) Perfect Bound on White w/Gloss Lam.
Language: English
Published by Springer, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
- Softcover
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Condition: New. PRINT ON DEMAND pp. 316.
Language: English
Published by Springer Netherlands, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
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Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Text no 1 Radio Recombination Lines (RRLs), discovered in the USSR in 1964, have become a powerful research tool for astronomers. Available throughout the radio spectrum, these lines carry information regarding the de…nsity, temperature, turbulence.
Language: English
Published by Springer Netherlands Sep 2011, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
- Softcover
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Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Text no 1 Radio Recombination Lines (RRLs), discovered in the USSR in 1964, have become a powerful research tool for astronomers. Available throughout the radio spectrum, these lines carry information regarding the density, temperat…ure, turbulence and velocity of thermal plasmas. Their very existance shows the presence of thermal gas. They also can carry information regarding magnetic fields if Zeeman splitting were to be detected. Containing the proceedings of an IAU Colloquium celebrating the 25th anniversary of their detection, this volume tells us what has happened since. It contains the story of the detection of RRLs and reviews of many areas of physics of the interstellargas from which stars form, HII regions excited by newly formed stars, planetary nebulae involving dying stars, and the structure of our Milky Way and other galaxies reflecting the large-scale morphology of the star formation process. In addition there is an article describing modern laboratory studies of Rydberg atoms to probe the basic physics of atomic structure, and articles describing the theory of collisions and radiation upon Rydberg atoms leading to observate effects to be used as diagnostic tools in astromony. This book focuses on the 25 years of astronomical research with radio recombination lines (RRLs) since their discovery in 1965. It covers a wide range of topics: papers dealing with research into Rydberg atoms both in the laboratory and in the interstellar medium of our galaxy and others; papers on the interaction of radiation and atomic systems, as well as with the effects of inadiabatic collisions between these atoms and both ions and electrons. It deals with astronomical observations of atoms with `diameters' ranging from 0.08 to 50 mum a size factor of 625. It deals with RRLs in absorption, in emission and as true masers. And it deals with plasmas with temperatures ranging from 10 to greater than 104 kelvins, and with an even greater range of volume densities. Much new work is reported, including low frequency RRLs discovered in 1980 and the maser RRLs from the star MWC349, discovered in 1989. The advent of aperture synthesis telescopes and large single-element telescopes have made possible RRL studies with high angular resolution. The sum total of the work reported here will make the volume a platform from which to search new horizons in RRL research. 316 pp. Englisch.
Language: English
Published by Springer, Springer Sep 2011, 2011
Series: Astrophysics and Space Science Library, Book 96 of 228. Book 96 of 228 - Astrophysics and Space Science Library
- Softcover
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Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -Text no 1Radio Recombination Lines (RRLs), discovered in the USSR in 1964, have become a powerful research tool for astronomers. Available throughout the radio spectrum, these lines carry information regarding the density, temperature,…turbulence and velocity of thermal plasmas. Their very existance shows the presence of thermal gas. They also can carry information regarding magnetic fields if Zeeman splitting were to be detected.Containing the proceedings of an IAU Colloquium celebrating the 25th anniversary of their detection, this volume tells us what has happened since. It contains the story of the detection of RRLs and reviews of many areas of physics of the interstellargas from which stars form, HII regions excited by newly formed stars, planetary nebulae involving dying stars, and the structure of our Milky Way and other galaxies reflecting the large-scale morphology of the star formation process. In addition there is an article describing modern laboratory studies of Rydberg atoms to probe the basic physics of atomic structure, and articles describing the theory of collisions and radiation upon Rydberg atoms leading to observate effects to be used as diagnostic tools in astromony.This book focuses on the 25 years of astronomical research with radio recombination lines (RRLs) since their discovery in 1965. It covers a wide range of topics: papers dealing with research into Rydberg atoms both in the laboratory and in the interstellar medium of our galaxy and others; papers on the interaction of radiation and atomic systems, as well as with the effects of inadiabatic collisions between these atoms and both ions and electrons. It deals with astronomical observations of atoms with `diameters' ranging from 0.08 to 50 mum a size factor of 625. It deals with RRLs in absorption, in emission and as true masers. And it deals with plasmas with temperatures ranging from 10 to greater than 104 kelvins, andwith an even greater range of volume densities.Much new work is reported, including low frequency RRLs discovered in 1980 and the maser RRLs from the star MWC349, discovered in 1989. The advent of aperture synthesis telescopes and large single-element telescopes have made possible RRL studies with high angular resolution. The sum total of the work reported here will make the volume a platform from which to search new horizons in RRL research.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 316 pp. Englisch.
Language: English
Published by Springer Netherlands Sep 2012, 2012
Series: Astrophysics and Space Science Library, Book 6 of 228. Book 6 of 228 - Astrophysics and Space Science Library
- Softcover
- Print on Demand
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Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Recombination lines at radio wavelengths have been - and still are - a pow erful tool for modern astronomy. For more than thirty years they have allowed astronomers to probe the gases from which stars form. They have even been detec…ted in the Sun. In addition, observations of these spectral lines facilitate basic research into the atom, in forms and environments that can only exist in the huge dimensions and extreme conditions of cosmic laboratories. We intend this book to serve as a tourist's guide to the world of Radio Recombination Lines. It contains three divisions: a history of their discovery, the physics of how they form and how their voyage to us influences their spectral profiles, and a description of their many astronomical contributions to date. The appendix includes supplementary calculations that may be useful to some astronomers. This material also includes tables of line frequencies from 12 MHz to 30THz (AlOJLm) as well as FORTRAN computer code to calculate the fine structure components of the lines, to evaluate radial matrix integrals, and to calculate the departure coefficients of hydrogen in a cosmic environment. It also describes how to convert observational to astrophysical units. The text includes extensive references to the literature to assist readers who want more details. 380 pp. Englisch.
