8 results
Globular cluster metallicities and distances from disentangling their RR Lyrae light curves
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- Journal:
- Proceedings of the International Astronomical Union / Volume 18 / Issue S376 / December 2022
- Published online by Cambridge University Press:
- 06 February 2024, pp. 222-238
- Print publication:
- December 2022
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RR Lyrae in M15: Fourier Decomposition and Physical Parameters
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- Journal:
- Proceedings of the International Astronomical Union / Volume 2 / Issue S240 / August 2006
- Published online by Cambridge University Press:
- 09 August 2007, pp. 605-612
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- August 2006
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Multisite observations of the pre–Main-Sequence $\delta$ Scuti star IP Per
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- Journal:
- Proceedings of the International Astronomical Union / Volume 2004 / Issue IAUS224 / July 2004
- Published online by Cambridge University Press:
- 02 March 2005, pp. 799-803
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- July 2004
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Activity as the Main Explanation of Light Variations of o And — Towards a Rotational Modulation Model
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- Journal:
- International Astronomical Union Colloquium / Volume 185 / 2002
- Published online by Cambridge University Press:
- 12 April 2016, pp. 238-239
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- 2002
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Optical Variability of the Be Star o And during the Period 1975–1998: Rotational Modulation or Multimodal Pulsations?
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- Journal:
- International Astronomical Union Colloquium / Volume 175 / 2000
- Published online by Cambridge University Press:
- 12 April 2016, pp. 205-207
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- 2000
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Supergiant Stars as Tracers of Galactic Chemical Composition
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- Journal:
- Symposium - International Astronomical Union / Volume 164 / 1995
- Published online by Cambridge University Press:
- 07 August 2017, p. 366
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- 1995
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On the Brightness and Pulsational Properties of Yellow Supergiants
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- Journal:
- International Astronomical Union Colloquium / Volume 82 / 1985
- Published online by Cambridge University Press:
- 12 April 2016, pp. 91-92
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- 1985
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On The Binary Nature of 89 Herculis
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- Journal:
- International Astronomical Union Colloquium / Volume 82 / 1985
- Published online by Cambridge University Press:
- 12 April 2016, pp. 81-82
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- 1985
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