... Jeremy Dietrich . Harvard . Howard Smith . SEDs of InteractingGalaxies . Callie Hood . UNC . Jayne Birkby . ... Lee Rosenthal . Haverford . Howard Smith . Late-Stage InteractingGalaxies . Peter Senchya . Wash.U . Matt Ashby, Joe Hora . ...
... Caltech . The Spitzer InteractingGalaxies Survey: IRAC Evaluations of Star Formation . ------- Text of final project abstract is not available. ...
... a) Big Bang model, because those galaxies are expanding towards us. $b) Local Group concept, because nearby galaxiesinteract gravitationally. c) evolution theory, because galaxies change color as they evolve. d) oscillating universe theory, because some ...
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Ссылки http://hea-www.harvard.edu/~pgreen/educ/PIAhandout_25jan02.pdf -- 113.2 Кб -- 25.01.2002 Похожие документы
... PROJECT TITLE: Evolving Physical Processes in Late-Stage InteractingGalaxies as Revealed through Mid-IR Photometry, Spectroscopy, and Galaxy Simulations . ...
... 2012, MNRAS, in press ``The jet-cloud interacting radio galaxy PKS B2152-699. I. Structures revealed in new deep radio and X-ray observations,'' . ...
... Strong soft X-ray emission from the galactic hot bubbles/winds is often found in the local merging/interactinggalaxies (e.g., the Antennae; Fabbiano et al. ...
... The long tail is formed by ram pressure stripping as M86 falls into the Virgo cluster of galaxies (off image to the lower left) and interacts with the Virgo ICM. ...
... 6 .3 .4 Angular Resolution An angular resolution (HPD) of 15 arcsec is required in order to separate IMBH from nearby bright point sources and diffuse emission in nearby (z<0.1) interactinggalaxies. ...
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Ссылки http://hea-www.harvard.edu/~garcia/conx/conx_srd_001008.pdf -- 258.4 Кб -- 28.06.2011 Похожие документы