Tīmeklis2015. gada 19. nov. · Authors: Rene Oudmaijer (Leeds, UK), Willem-Jan de Wit (ESO, Chile) Download PDF Abstract: This chapter discusses the use and possibilities of optical and infrared interferometry to study star formation. The chapter starts with a brief overview of the star formation process and highlights the open questions from an … Tīmeklis2015. gada 14. sept. · Professor Rene Oudmaijer, a co-author of the study, also from the University’s School of Physics and Astronomy, said: “Considering the large distance that separates us from the star (325 light-years), the challenge was similar to trying to observe something the size of a pinhead from 100km away.”
Rene Oudmaijer IAU - International Astronomical Union
Professor Rene Oudmaijer Position: Professor Areas of expertise: star formation; pre-main sequence evolution; stellar evolution; circumstellar matter; binary stars; interferometry. Email: [email protected] Phone: +44 (0)113 343 3886 Website: Papers Profile My research concerns the formation of … Skatīt vairāk My research concerns the formation of stars. In particular, I investigate the accretion of matter onto the star until it reaches its final … Skatīt vairāk My research interests concern the formation of stars, their circumstellar disks and stellar evolution in general. I study these using complementary observational approaches. On the one hand I study larger samples of … Skatīt vairāk Tīmeklis2008. gada 23. jūl. · Authors: Rene Oudmaijer (Leeds, UK), Andrew Parr (Leeds), Deborah Baines (NPL, Leeds), John Porter (Liverpool John Moores, UK) finance and the preservation of wealth
Astronomers Discover Closest High-Mass Stellar Objects
Tīmeklis0. 22 views 6 months ago. IR2024 René Oudmaijer University of Leeds Day Five Session Two Multiple mass loss events on timescales of hundreds of years of the … Tīmeklis2012. gada 19. dec. · Authors: Rene Oudmaijer (Leeds), Willem-Jan de Wit (ESO) Download PDF Abstract: IRC +10420 is one of the few known massive stars in rapid transition from the Red Supergiant phase to the Wolf-Rayet or Luminous Blue Variable phase. The star has an ionised wind and using the Br gamma hydrogen … Tīmeklis2 Rene´ Oudmaijer proceedings, spectropolarimetry is a very powerful method to probe circumstellar ma-terial close to a star. It takes advantage of the fact that due to collisions with electrons in an ionized medium, the light from the star is much more polarized than the emission lines such as Hαwhich originate from the gas itself. finance and thrift fresno