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- Table 7: NGC 5987 Minor Axis (PA --29) Radius R \Sigma B \Gamma R \Sigma U \Gamma R \Sigma R \Gamma K \Sigma R \Gamma I \Sigma J \Gamma K \Sigma
- F32AA4 The Structure of Stars 1. The nuclear reaction rate in a particular kind of star is proportional to
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- Table 10: NGC 5987 Isophote Shapes Radius K \Sigma ffl (1 b
- Table 9: NGC 5987 Major Axis Radius R \Sigma B \Gamma R \Sigma U \Gamma R \Sigma R \Gamma K \Sigma R \Gamma I \Sigma J \Gamma K \Sigma
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- Table 8: NGC 5326 Minor Axis (D) (PA --42) Radius R \Sigma B \Gamma R \Sigma U \Gamma R \Sigma R \Gamma K \Sigma R \Gamma I \Sigma J \Gamma K \Sigma
- Table 7: IC 1029 Minor Axis (PA --119) Radius R \Sigma B \Gamma R \Sigma U \Gamma R \Sigma R \Gamma K \Sigma R \Gamma I \Sigma U \Gamma K \Sigma
- Session Huug and the KNVWSSession Huug and the KNVWS The Young Huug van WoerdenThe Young Huug van Woerden
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- Table 9: NGC 5326 Major Axis Radius R \Sigma B \Gamma R \Sigma U \Gamma R \Sigma R \Gamma K \Sigma R \Gamma I \Sigma J \Gamma K \Sigma
- Table 8: NGC 5707 Minor Axis (D) (PA 121) Radius R \Sigma B \Gamma R \Sigma U \Gamma R \Sigma R \Gamma K \Sigma R \Gamma I \Sigma U \Gamma K \Sigma
- H.J. Woertche Basic Detection Techniques 2006
- F32AA4 The Structure of Stars Solutions 6
- Table 10: NGC 5689 Isophote Shapes Radius K \Sigma ffl (1 b
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- Table 10: NGC 5326 Isophote Shapes Radius K \Sigma ffl (1 b
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- Detection of energetic particles and gamma rays The interaction of radiation with matter
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- 1.Basic Properties of Stars This is the Sun during a total eclipse. The Sun, our closest star, is very much
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- 5. Energy Production and Transport 5.1 Energy Release from Nuclear Reactions
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- 8. The evolution of stars a more detailed picture 8.1Pre Main-Sequence Evolution
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- NASSP OT1: Telescopes I-217 Feb 2010 1 Optical/IR Observational Astronomy
- NASSP OT1: Telescopes II-119 Feb 2010 1 Optical/IR Observational Astronomy
- THE OPTICAL-INFRARED WAVELENGTH DOMAIN
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- NASSP OT1: Detectors I24 Feb 2010 1 Optical/IR Observational Astronomy
- NASSP OT1: Detectors II26 Feb 2010 1 Optical/IR Observational Astronomy
- OT1: Detectors III CCDs1 March 2010 1 Optical/IR Observational Astronomy
- Recollection 1965-1971: The Groningen High Latitude Survey
- Interstellar Absorption Lines and the Halo
- Centre of Excellence in Evolutionary Cosmology The Search for HI Clouds in Local Group Analogs
- Jacobus Kapteyn (1851-1922) Astronomical Databases and the VO
- F32AA4 The Structure of Stars Solutions 5
- Table 9: NGC 5689 Major Axis Radius R \Sigma B \Gamma R \Sigma U \Gamma R \Sigma R \Gamma K \Sigma R \Gamma I \Sigma J \Gamma K \Sigma
- Distances toDistances to HVCsHVCs usingusing blue horizontal branch starsblue horizontal branch stars
- 4.Polytropes 4.1Definitions
- Statistical Analysis of CCD Data: Error Analysis/Noise Theorem
- Publications in refereed journals 115. Krajnovic, D., ..., Peletier, R.F., et al. 2008, MNRAS, 390, 93
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- b) intensity changes: scintillation !I/I on the ground is proportional to h !", i.e. # he-h/H
- IV DETECTORS up to 1837: HUMAN EYE + : relatively high Q.E. (~10%),
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