Photometric Investigations Of Several Early
Photometric Investigations Of Several Early - Doğuş Özuyar
Chapter 1: Introduction
1.1. Variable Stars
1.2. Intrinsic Variable Stars
1.3. Extrinsic Variable Stars
Chapter 2: Solar TErrestrial RElations Observatory (STEREO)
2.1. STEREO Data and Reduction Procedures
Chapter 3: ANALysıs TECHNIQUES of NUMERICAL DATA
3.1. Introduction
3.2. Lomb-Scargle Periodogram (LS)
3.3. Phase Dispersion Minimization (PDM)
3.4. Period04
3.5. Wavelet Transforms
3.6. Discussion
Chapter 4: Frequency ANALYSeS of synthetic lıght curves
4.1. Introduction
4.2. Noise Types
4.3. The Auto-correlation Function
4.4. Synthetic Light Curves
4.5. Results
4.6. Discussion
Chapter 5: PerIOD evolutıon of some chemically peculıar STARS
5.1. Introduction
5.2. Analysis of STEREO Data
5.3. Other Procedures
5.4. Target Selection
5.5. Results
5.6. Discussion
Chapter 6: Photometric and spectroscopic evolution of some brıght be-stars: the relatıon between non-radıal pulsatıons and dısk structures
6.1. Introduction
6.2. Selection of Be-Star Samples
6.3. Data Analysis
6.4. Results
6.5. Discussion
Chapter 7: Pulsatıonal Characteristıcs Of A Sample Of Scutı Stars And Theır Relatıons Between Stellar Parameters
7.1. Introduction
7.2. Analysis of STEREO Data
7.3. STEREO Samples of δ Scuti Stars
7.4. Results
7.5. Discussion
Chapter 8: Overview And Future Work
(Tanıtım Bülteninden)
Photometric Investigations Of Several Early - Doğuş Özuyar
Chapter 1: Introduction
1.1. Variable Stars
1.2. Intrinsic Variable Stars
1.3. Extrinsic Variable Stars
Chapter 2: Solar TErrestrial RElations Observatory (STEREO)
2.1. STEREO Data and Reduction Procedures
Chapter 3: ANALysıs TECHNIQUES of NUMERICAL DATA
3.1. Introduction
3.2. Lomb-Scargle Periodogram (LS)
3.3. Phase Dispersion Minimization (PDM)
3.4. Period04
3.5. Wavelet Transforms
3.6. Discussion
Chapter 4: Frequency ANALYSeS of synthetic lıght curves
4.1. Introduction
4.2. Noise Types
4.3. The Auto-correlation Function
4.4. Synthetic Light Curves
4.5. Results
4.6. Discussion
Chapter 5: PerIOD evolutıon of some chemically peculıar STARS
5.1. Introduction
5.2. Analysis of STEREO Data
5.3. Other Procedures
5.4. Target Selection
5.5. Results
5.6. Discussion
Chapter 6: Photometric and spectroscopic evolution of some brıght be-stars: the relatıon between non-radıal pulsatıons and dısk structures
6.1. Introduction
6.2. Selection of Be-Star Samples
6.3. Data Analysis
6.4. Results
6.5. Discussion
Chapter 7: Pulsatıonal Characteristıcs Of A Sample Of Scutı Stars And Theır Relatıons Between Stellar Parameters
7.1. Introduction
7.2. Analysis of STEREO Data
7.3. STEREO Samples of δ Scuti Stars
7.4. Results
7.5. Discussion
Chapter 8: Overview And Future Work
(Tanıtım Bülteninden)
Taksit Sayısı | Taksit tutarı | Genel Toplam |
---|---|---|
1 | - | - |
2 | 120,75 | 241,50 |
3 | 86,14 | 258,41 |
4 | - | - |
6 | 44,68 | 268,07 |
9 | 30,72 | 276,52 |
Taksit Sayısı | Taksit tutarı | Genel Toplam |
---|---|---|
1 | - | - |
2 | 120,75 | 241,50 |
3 | 89,11 | 267,34 |
4 | - | - |
6 | 44,28 | 265,65 |
9 | 30,72 | 276,52 |
Taksit Sayısı | Taksit tutarı | Genel Toplam |
---|---|---|
1 | - | - |
2 | 120,75 | 241,50 |
3 | 86,14 | 258,41 |
4 | - | - |
6 | 44,28 | 265,65 |
9 | 30,72 | 276,52 |
Taksit Sayısı | Taksit tutarı | Genel Toplam |
---|---|---|
1 | - | - |
2 | 120,75 | 241,50 |
3 | 86,14 | 258,41 |
4 | - | - |
6 | 44,48 | 266,86 |
9 | 30,72 | 276,52 |
Taksit Sayısı | Taksit tutarı | Genel Toplam |
---|---|---|
1 | - | - |
2 | 120,75 | 241,50 |
3 | 86,14 | 258,41 |
4 | 65,81 | 263,24 |
6 | 44,28 | 265,65 |
9 | 30,72 | 276,52 |
Taksit Sayısı | Taksit tutarı | Genel Toplam |
---|---|---|
1 | - | - |
2 | 120,75 | 241,50 |
3 | 86,14 | 258,41 |
4 | - | - |
6 | 44,28 | 265,65 |
9 | 30,72 | 276,52 |
Taksit Sayısı | Taksit tutarı | Genel Toplam |
---|---|---|
Tek Çekim | 241,50 | 241,50 |
2 | 120,75 | 241,50 |
3 | 86,14 | 258,41 |
4 | - | - |
6 | 44,28 | 265,65 |
9 | 30,86 | 277,73 |