Amplitude Modulation of Pulsation Modes in Delta Scuti Stars
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Preise | 2017 | 2019 | 2020 |
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Schnitt | Fr. 146.60 (€ 149.79)¹ | Fr. 127.51 (€ 130.29)¹ | Fr. 147.62 (€ 150.83)¹ |
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1
Amplitude Modulation of Pulsation Modes in Delta Scuti Stars (2017)
~EN HC NW
ISBN: 9783319666488 bzw. 3319666487, vermutlich in Englisch, Springer, Berlin Springer International Publishing, gebundenes Buch, neu.
Lieferung aus: Deutschland, Versandkosten nach: Deutschland, Versandkostenfrei.
Von Händler/Antiquariat, buecher.de GmbH & Co. KG, [1].
This outstanding thesis by Dominic Bowman provides a thorough investigation of long-standing questions as to whether amplitude modulation is astrophysical, whether it offers insights into pulsating stars, and whether simple beating of modes with stable amplitudes is unrecognised because of a lack of frequency resolution. In this thesis, the author studied a uniform sample of 983 delta Scuti stars-the most common type of main-sequence heat engine pulsator-that were observed nearly continuously for 4 years at stunning photometric precision of only a few parts per million by the Kepler space mission. With no mission planned to supersede the Kepler 4-year data set, this thesis will stand as the definitive study of these questions for many years. With revolutionary photometric data from the planet-hunting Kepler space mission, asteroseismic studies have been carried out on many hundreds of main-sequence solar-type stars and about 10,000 red giants. It is easy to understand why those stochastically driven stars have highly variable amplitudes. Over much of the rest of the Hertzsprung-Russell (HR) diagram, stellar pulsations are driven by heat mechanisms, which are much more regular than the stochastic driving in solar-like pulsators. Yet for decades, amplitude and frequency modulation of pulsation modes have been observed in almost all types of heat-driven pulsating stars. The author shows that the amplitude and frequency modulation are astrophysical, and he has investigated their implications and prospects to provide new insights into the delta Scuti stars and the many other types of heat-engine pulsators across the HR diagram. 1st ed. 2017. 2017. xvi, 204 S. 21 SW-Abb., 62 Farbabb. 235 mm Versandfertig in 3-5 Tagen, Hardcover, Neuware, Offene Rechnung (Vorkasse vorbehalten).
Von Händler/Antiquariat, buecher.de GmbH & Co. KG, [1].
This outstanding thesis by Dominic Bowman provides a thorough investigation of long-standing questions as to whether amplitude modulation is astrophysical, whether it offers insights into pulsating stars, and whether simple beating of modes with stable amplitudes is unrecognised because of a lack of frequency resolution. In this thesis, the author studied a uniform sample of 983 delta Scuti stars-the most common type of main-sequence heat engine pulsator-that were observed nearly continuously for 4 years at stunning photometric precision of only a few parts per million by the Kepler space mission. With no mission planned to supersede the Kepler 4-year data set, this thesis will stand as the definitive study of these questions for many years. With revolutionary photometric data from the planet-hunting Kepler space mission, asteroseismic studies have been carried out on many hundreds of main-sequence solar-type stars and about 10,000 red giants. It is easy to understand why those stochastically driven stars have highly variable amplitudes. Over much of the rest of the Hertzsprung-Russell (HR) diagram, stellar pulsations are driven by heat mechanisms, which are much more regular than the stochastic driving in solar-like pulsators. Yet for decades, amplitude and frequency modulation of pulsation modes have been observed in almost all types of heat-driven pulsating stars. The author shows that the amplitude and frequency modulation are astrophysical, and he has investigated their implications and prospects to provide new insights into the delta Scuti stars and the many other types of heat-engine pulsators across the HR diagram. 1st ed. 2017. 2017. xvi, 204 S. 21 SW-Abb., 62 Farbabb. 235 mm Versandfertig in 3-5 Tagen, Hardcover, Neuware, Offene Rechnung (Vorkasse vorbehalten).
2
Amplitude Modulation of Pulsation Modes in Delta Scuti Stars
DE NW EB
ISBN: 9783319666488 bzw. 3319666487, in Deutsch, Springer International Publishing, neu, E-Book.
Lieferung aus: Vereinigte Staaten von Amerika, E-Book zum download.
Science, This outstanding thesis by Dominic Bowman provides a thorough investigation of long-standing questions as to whether amplitude modulation is astrophysical, whether it offers insights into pulsating stars, and whether simple beating of modes with stable amplitudes is unrecognised because of a lack of frequency resolution. In this thesis, the author studied a uniform sample of 983 delta Scuti starsthe most common type of main-sequence heat engine pulsatorthat were observed nearly continuously for 4 years at stunning photometric precision of only a few parts per million by the Kepler space mission. With no mission planned to supersede the Kepler 4-year data set, this thesis will stand as the definitive study of these questions for many years. With revolutionary photometric data from the planet-hunting Kepler space mission, asteroseismic studies have been carried out on many hundreds of main-sequence solar-type stars and about 10,000 red giants. It is easy to understand why those stochastically driven stars have highly variable amplitudes. Over much of the rest of the HertzsprungRussell (HR) diagram, stellar pulsations are driven by heat mechanisms, which are much more regular than the stochastic driving in solar-like pulsators. Yet for decades, amplitude and frequency modulation of pulsation modes have been observed in almost all types of heat-driven pulsating stars. The author shows that the amplitude and frequency modulation are astrophysical, and he has investigated their implications and prospects to provide new insights into the delta Scuti stars and the many other types of heat-engine pulsators across the HR diagram. eBook.
Science, This outstanding thesis by Dominic Bowman provides a thorough investigation of long-standing questions as to whether amplitude modulation is astrophysical, whether it offers insights into pulsating stars, and whether simple beating of modes with stable amplitudes is unrecognised because of a lack of frequency resolution. In this thesis, the author studied a uniform sample of 983 delta Scuti starsthe most common type of main-sequence heat engine pulsatorthat were observed nearly continuously for 4 years at stunning photometric precision of only a few parts per million by the Kepler space mission. With no mission planned to supersede the Kepler 4-year data set, this thesis will stand as the definitive study of these questions for many years. With revolutionary photometric data from the planet-hunting Kepler space mission, asteroseismic studies have been carried out on many hundreds of main-sequence solar-type stars and about 10,000 red giants. It is easy to understand why those stochastically driven stars have highly variable amplitudes. Over much of the rest of the HertzsprungRussell (HR) diagram, stellar pulsations are driven by heat mechanisms, which are much more regular than the stochastic driving in solar-like pulsators. Yet for decades, amplitude and frequency modulation of pulsation modes have been observed in almost all types of heat-driven pulsating stars. The author shows that the amplitude and frequency modulation are astrophysical, and he has investigated their implications and prospects to provide new insights into the delta Scuti stars and the many other types of heat-engine pulsators across the HR diagram. eBook.
3
Symbolbild
Amplitude Modulation of Pulsation Modes in Delta Scuti Stars (2017)
~EN HC NW
ISBN: 9783319666488 bzw. 3319666487, vermutlich in Englisch, Springer International Publishing AG, Cham, gebundenes Buch, neu.
Lieferung aus: Vereinigte Staaten von Amerika, zzgl. Versandkosten, Versandgebiet: STOCKNEW.
Von Händler/Antiquariat, Alibris, NV, Sparks, [RE:5].
Hard cover.
Von Händler/Antiquariat, Alibris, NV, Sparks, [RE:5].
Hard cover.
4
Symbolbild
Amplitude Modulation of Pulsation Modes in Delta Scuti Stars (2017)
~EN HC NW FE
ISBN: 9783319666488 bzw. 3319666487, vermutlich in Englisch, Springer, gebundenes Buch, neu, Erstausgabe.
Lieferung aus: Vereinigtes Königreich Grossbritannien und Nordirland, zzgl. Versandkosten, Versandgebiet: EUR.
Von Händler/Antiquariat, Paperbackshop International, GLOS, Fairford, [RE:4].
Hardcover, 1st ed. 2017.
Von Händler/Antiquariat, Paperbackshop International, GLOS, Fairford, [RE:4].
Hardcover, 1st ed. 2017.
5
Symbolbild
Amplitude Modulation of Pulsation Modes in Delta Scuti Stars (2017)
~EN HC NW FE
ISBN: 9783319666488 bzw. 3319666487, vermutlich in Englisch, Springer, gebundenes Buch, neu, Erstausgabe.
Lieferung aus: Vereinigtes Königreich Grossbritannien und Nordirland, zzgl. Versandkosten, Versandgebiet: EUR.
Von Händler/Antiquariat, Books2anywhere, GLOUCESTERSHIRE, Fairford, [RE:4].
Hardcover, 1st ed. 2017.
Von Händler/Antiquariat, Books2anywhere, GLOUCESTERSHIRE, Fairford, [RE:4].
Hardcover, 1st ed. 2017.
6
Symbolbild
Amplitude Modulation of Pulsation Modes in Delta Scuti Stars (Springer Theses) (2017)
~DE HC NW
ISBN: 9783319666488 bzw. 3319666487, vermutlich in Deutsch, Springer, gebundenes Buch, neu.
Lieferung aus: Vereinigtes Königreich Grossbritannien und Nordirland, zzgl. Versandkosten, Versandgebiet: EUR.
Von Händler/Antiquariat, AwesomeBooksUK, OXON, PO BOX 318, [RE:4].
Hardcover.
Von Händler/Antiquariat, AwesomeBooksUK, OXON, PO BOX 318, [RE:4].
Hardcover.
7
Symbolbild
Amplitude Modulation of Pulsation Modes in Delta Scuti Stars (Springer Theses) (2017)
~EN HC NW
ISBN: 9783319666488 bzw. 3319666487, vermutlich in Englisch, Springer, gebundenes Buch, neu.
Lieferung aus: Vereinigte Staaten von Amerika, zzgl. Versandkosten, Versandgebiet: DOM.
Von Händler/Antiquariat, Awesomebooks_Newbooks, DE, Wilmington, [RE:4].
Hardcover.
Von Händler/Antiquariat, Awesomebooks_Newbooks, DE, Wilmington, [RE:4].
Hardcover.
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