... unknown low-mass (giant planet and brown dwarf) companions to stars in the solar ... A systematic survey of nearby stars for giant planet and brown dwarf companions, and ...
... where the old low mass stars on the red giant branch evolutionary phase are more ... the red supergiants (RSGs) but barely reach the asymptotic giant branch (AGB) stars ...
... image brown dwarfs or giant planets around main-sequence stars is the overwhelming ... binary distribution of stars as well as the average distance of the giant planets in ...
... analysis of the data reveals a color magnitude diagram with both a clump of blue stars with the correct properties to be the tip of the main sequence and a clump of red stars which are likely to be red giants, another population expected at the Center ...
... emission from individual asymptotic giant branch stars in the Magellanic Clouds ... topic is the search for continuum radio emission from red giant and supergiant stars ...
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Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf -- 1000.5 Кб -- 04.09.2008 Похожие документы
... the VLTI or SIM; (d) stars with detected giant planets exhibit an impressive excess ... complete a census of gas and ice giants around stars of all masses; (d) detection of ...
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Ссылки http://www.stecf.org/coordination/esa_eso/extrasolar/report.pdf -- 1083.5 Кб -- 04.09.2008 Похожие документы
... IRC10216, a nearby carbon star ESA-ESO Meeting, Feb 10-11, 2005 Solar System Objects Herschel can easily measure outer planets, and moons of these planets, as well as Trans Neptune Objects Highly accurate photometry Water on the giant planets and comets ...
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Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/esa-feb11-05-ver4.pdf -- 2622.1 Кб -- 04.09.2008 Похожие документы
... The Evolution of Stars seen with ISOCAM - the Need for NICMOS and VLT Follow Up. Abstract: . Introduction . ... 1 sees the process of stellar evolution. i) Standard staring and coronographic observations with ISOCAM towards BD+31 643 are ...
... Kobayashi et al. (1998) assume two SD scenarios for companion stars, one involving a red-giant companion with MRG;0 1M , and one with a main- sequence star with MMS;0 2 3 M . ...
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Ссылки http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/strolger04.ps -- 1023.9 Кб -- 16.09.2004 Похожие документы