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1. Astronomy HyperText Book: Stellar Evolution
... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...
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Ссылки http://zebu.uoregon.edu/textbook/se.html -- 4.8 Кб -- 16.12.1997
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2. Our group
... She is working with Claus Leitherer on different properties of the star formation process in local irregular galaxies. ... Her main research interests involve: the role of evolution in galaxy properties; the environmental effects in galaxy evolution/formation; the properties of star-forming galaxies at low and high redshifts; the starburst/AGN connection. ... She is working with Daniela Calzetti, Claus Leitherer, and Tim Heckman on the structure and evolution of starburst galaxies. ...
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Ссылки http://www.stsci.edu/science/starburst/our-group.html -- 9.4 Кб -- 13.10.2003
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3. http://www.eso.org/~hboffin/Astronet/Presentations/Panel_C.pdf
... Poitiers, 23 January 2007 Science Vision for European Astronomy in the Next 20 Years 2 Is the initial mass function universal? ... High Poitiers, 23 January 2007 Science Vision for European Astronomy in the Next 20 Years 4 Do we understand stellar structure and evolution? ... Interferometry in near infrared and radio: measuring radii and resolving stellar surface Science Vision for European Astronomy in the Next 20 Years Poitiers, 23 January 2007 5 What is the life-cycle of the ISM and Stars? ...
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Ссылки http://www.eso.org/~hboffin/Astronet/Presentations/Panel_C.pdf -- 714.8 Кб -- 31.01.2007
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4. EXTREME HELIUM STARS
Next: STELLAR PROPERTIES Up: EXTREME HELIUM STARS: PULSATION Previous: EXTREME HELIUM STARS: PULSATION . ... The latter are distributed over most of the Hertzsprung-Russell diagram; one of the most extreme examples is provided by the extreme helium stars (EHes) - early-type supergiants practically void of hydrogen in their atmospheres. ... Next: STELLAR PROPERTIES Up: EXTREME HELIUM STARS: PULSATION Previous: EXTREME HELIUM STARS: PULSATION Simon Jeffery . ...
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Ссылки http://star.arm.ac.uk/~csj/research/ehe_review/node1.html -- 6.1 Кб -- 25.01.2002
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5. High-resolution Herschel spectroscopy reveals the proto-planetary disk around
... High-resolution Herschel spectroscopy reveals the proto-planetary disk around the young star T Tau N . ... A study led by Linda Podio ( AstroFIt fellow at the Arcetri Observatory) with Inga Kamp (Kapteyn Institute, the Netherlands), Claudio Codella (Observatory of Arcetri) and other collaborators from Grenoble, UK and USA, makes use of high-resolution spectroscopic observations with HIFI on board the Herschel space observatory to characterize the disk around the young star T Tau N . ...
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Ссылки http://www.arcetri.astro.it/en/previous/204-scientific-news/713-ttaundisk -- 26.2 Кб -- 10.04.2016
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6. <