標(biāo)題: Titlebook: Amplitude Modulation of Pulsation Modes in Delta Scuti Stars ; Dominic M. Bowman Book 2017 Springer International Publishing AG 2017 Delta [打印本頁] 作者: patch-test 時間: 2025-3-21 18:18
書目名稱Amplitude Modulation of Pulsation Modes in Delta Scuti Stars 影響因子(影響力)
書目名稱Amplitude Modulation of Pulsation Modes in Delta Scuti Stars 影響因子(影響力)學(xué)科排名
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書目名稱Amplitude Modulation of Pulsation Modes in Delta Scuti Stars 網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Amplitude Modulation of Pulsation Modes in Delta Scuti Stars 被引頻次
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書目名稱Amplitude Modulation of Pulsation Modes in Delta Scuti Stars 讀者反饋
書目名稱Amplitude Modulation of Pulsation Modes in Delta Scuti Stars 讀者反饋學(xué)科排名
作者: 觀察 時間: 2025-3-21 21:39
Springer Theseshttp://image.papertrans.cn/a/image/154756.jpg作者: mydriatic 時間: 2025-3-22 00:53 作者: 和平 時間: 2025-3-22 04:57 作者: 愛國者 時間: 2025-3-22 12:43 作者: 配置 時間: 2025-3-22 14:42 作者: Misgiving 時間: 2025-3-22 20:52
Viertes Kapitel: Anleihepolitik,escope provided high photometric precision, a high duty cycle and data spanning four years for approximately 200 000 stars. In this chapter, a review of the .Space Telescope is provided including relevant details of using .data for asteroseismology. Also, the processing of all .observations of A and作者: Deject 時間: 2025-3-22 21:41
Viertes Kapitel: Anleihepolitik,ion mode exhibits amplitude modulation in KIC?7106205 whilst all other pulsation modes remain constant in amplitude, such that the visible pulsation energy budget is not conserved over the 4-yr .?data set. In this chapter, the published results from the analysis of this . Scuti star are discussed an作者: 小平面 時間: 2025-3-23 01:45 作者: recede 時間: 2025-3-23 08:03 作者: 游行 時間: 2025-3-23 12:40
Heldentotenfeiern in der deutschen Musikodels providing no predictive power of pulsation mode amplitudes. In this chapter, the non-linearity of pulsations in . Sct and gamma Dor stars is investigated, which includes the application of mode coupling models to determine the strength of non-linearity in a selection of pulsating stars. Furthe作者: 衍生 時間: 2025-3-23 15:56
Johann Sebastian Bach und der Krieg3 mag and predominantly pulsate in the fundamental and/or first overtone radial p modes. These stars are rare, making up less than one per cent of pulsating stars in the classical instability strip. In this chapter, the only two HADS stars observed by the . Space Telescope are studied, including det作者: 破譯 時間: 2025-3-23 21:49
Preu?en- und Hohenzollern-Lieder von Loeweemble of 983 stars that were observed continuously for four years at an unprecedented level of photometric precision. A search for amplitude modulation in these stars showed that the majority exhibit amplitude modulation in at least a single pulsation mode. Thus, timescales of years and longer are s作者: deadlock 時間: 2025-3-23 22:59
Amplitude Modulation of Pulsation Modes in Delta Scuti Stars 978-3-319-66649-5Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: palliative-care 時間: 2025-3-24 05:54
Viertes Kapitel: Anleihepolitik,ommon type of pulsator among main sequence A and F stars, and are found in a transition region between low- and high-mass stars in the HR?diagram. The hybrid stars found in the . data set and an evaluation of the observational blue and red edges of the classical instability strip are also discussed.作者: Hangar 時間: 2025-3-24 09:10 作者: 信條 時間: 2025-3-24 11:32 作者: 拋射物 時間: 2025-3-24 17:44 作者: 白楊 時間: 2025-3-24 20:02 作者: 撫慰 時間: 2025-3-25 02:06
Heldentotenfeiern in der deutschen Musikestigated, which includes the application of mode coupling models to determine the strength of non-linearity in a selection of pulsating stars. Furthermore, a method to distinguish combination frequencies and coupled pulsation modes and its implications are discussed.作者: Absenteeism 時間: 2025-3-25 06:51
Johann Sebastian Bach und der Kriegsating stars in the classical instability strip. In this chapter, the only two HADS stars observed by the . Space Telescope are studied, including detectable changes in pulsation mode periods that may be caused by stellar evolution.作者: 舔食 時間: 2025-3-25 07:48
The , Space Photometry Revolution,of the .Space Telescope is provided including relevant details of using .data for asteroseismology. Also, the processing of all .observations of A and F stars is discussed, which formed the data set to find all the delta Sct stars studied in this monograph.作者: 山崩 時間: 2025-3-25 13:53 作者: COW 時間: 2025-3-25 19:42
Amplitude Modulation in , Delta Scuti Stars, mode amplitudes, amplitude modulation caused by beating, and amplitude modulation caused by non-linearity. It is shown that the majority of .?Sct stars observed by . exhibit amplitude modulation in at least one pulsation mode, and the observational and physical implications of this are discussed.作者: 初學(xué)者 時間: 2025-3-25 21:12 作者: 消滅 時間: 2025-3-26 03:00
Investigating the HADS Stars with , Data,sating stars in the classical instability strip. In this chapter, the only two HADS stars observed by the . Space Telescope are studied, including detectable changes in pulsation mode periods that may be caused by stellar evolution.作者: Guaff豪情痛飲 時間: 2025-3-26 04:39
Book 2017ical, 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 作者: 鳥籠 時間: 2025-3-26 10:22
,Chirurgische An?sthesie im Felde, modulation. Finally, an example of a well-studied delta Scuti star with known amplitude modulation is given, which demonstrates the diverse range of behaviour in these stars and motivated the results and conclusions presented in this monograph.作者: fructose 時間: 2025-3-26 13:24 作者: NAUT 時間: 2025-3-26 16:49
Preu?en- und Hohenzollern-Lieder von Loewering within a star. The observational studies of individual stars in this monograph provide strong evidence that non-linear processes are clearly at work in the many . Sct stars and provide valuable constraints for future asteroseismic modelling.作者: Mettle 時間: 2025-3-27 00:09
Conclusions and Future Work,ring within a star. The observational studies of individual stars in this monograph provide strong evidence that non-linear processes are clearly at work in the many . Sct stars and provide valuable constraints for future asteroseismic modelling.作者: Glutinous 時間: 2025-3-27 03:51 作者: Cougar 時間: 2025-3-27 07:32 作者: 剝削 時間: 2025-3-27 13:17
Book 2017in-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 作者: vasospasm 時間: 2025-3-27 17:00 作者: 無法破譯 時間: 2025-3-27 18:00
Introduction, Eddington, the observation and modelling of stellar pulsations, which is known as asteroseismology, has been applied to many different types of stars in the HR diagram, covering a wide range in stellar mass and evolution. In this introduction chapter, overviews of asteroseismology, stellar pulsatio作者: gene-therapy 時間: 2025-3-28 00:26 作者: 異端 時間: 2025-3-28 05:13
,KIC?7106205 — An Archetypal Delta Scuti Star with Amplitude Modulation,ion mode exhibits amplitude modulation in KIC?7106205 whilst all other pulsation modes remain constant in amplitude, such that the visible pulsation energy budget is not conserved over the 4-yr .?data set. In this chapter, the published results from the analysis of this . Scuti star are discussed an作者: adroit 時間: 2025-3-28 09:19
, Observations of Delta Scuti Stars,ommon type of pulsator among main sequence A and F stars, and are found in a transition region between low- and high-mass stars in the HR?diagram. The hybrid stars found in the . data set and an evaluation of the observational blue and red edges of the classical instability strip are also discussed.作者: 不易燃 時間: 2025-3-28 13:14
Amplitude Modulation in , Delta Scuti Stars,able pulsation mode amplitudes can be grouped as intrinsic or extrinsic. Case study examples are given which demonstrate different scenarios: constant mode amplitudes, amplitude modulation caused by beating, and amplitude modulation caused by non-linearity. It is shown that the majority of .?Sct sta作者: recession 時間: 2025-3-28 18:11
Characterising Pulsational Non-linearity,odels providing no predictive power of pulsation mode amplitudes. In this chapter, the non-linearity of pulsations in . Sct and gamma Dor stars is investigated, which includes the application of mode coupling models to determine the strength of non-linearity in a selection of pulsating stars. Furthe作者: Statins 時間: 2025-3-28 18:50
Investigating the HADS Stars with , Data,3 mag and predominantly pulsate in the fundamental and/or first overtone radial p modes. These stars are rare, making up less than one per cent of pulsating stars in the classical instability strip. In this chapter, the only two HADS stars observed by the . Space Telescope are studied, including det作者: Generic-Drug 時間: 2025-3-29 00:45 作者: RAFF 時間: 2025-3-29 05:11
