Ðåíòãåíîâñêîå èçëó÷åíèå ãàëàêòèê â ëîêàëüíîé Âñåëåííîé è íà êîñìîëîãè÷åñêèõ êðàñíûõ ñìåùåíèÿõ. ... Ðàáîòû öèêëà ïîñâÿùåíû èññëåäîâàíèþ ðåíòãåíîâñêîãî èçëó÷åíèÿ îò çâåçäîîáðàçóþùèõ ãàëàêòèê â ëîêàëüíîé Âñåëåííîé è íà êîñìîëîãè÷åñêèõ êðàñíûõ ñìåùåíèÿõ. ... Ñðàâíåíèå ýòèõ äâóõ âåëè÷èí ïîêàçûâàåò , ÷òî óäåëüíàÿ ðåíòãåíîâñêàÿ ñâåòèìîñòü L X / SFR çâåçäîîáðàçóþùèõ ãàëàêòèê íà êîñìîëîãè÷åñêèõ êðàñíûõ ñìåùåíèÿõ íå ìîãëà çàìåòíî ïðåâûøàòü ëîêàëüíîå çíà÷åíèå - íå áîëåå ÷åì â 2 ðàçà íà êðàñíûõ ñìåùåíèÿõ z ˜2. ...

Welcome to the Starburst and Galaxy Evolution website.

... 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. ...

... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Late Stages of Stellar Evolution . Welcome to the home page of the Late Stages of Stellar Evolution" We are a research group which operates within the Astrophysics Group of the Australia Telescope National Facility. ... To investigate the late stages of stellar evolution and in particular the role of stellar mass-loss in the evolution of asymptotic giant branch stars, proto-planetary nebulae and extremely massive stars. ...

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

Next: The Supernovae Rates Up: No Title Previous: Gravitational wave background from . In this Section we present the results of the Scenario Machine simulation of supernova explosion (SN) rates in the Galaxy for various types of supernovae and apply them for estimating the - dependence for the SN in the Universe (see JÆrgensen et al. 1995[ 80 ]). The Supernovae Rates . Dependence for the Supernova Explosions . for Supernova Explosions . Results and Discussion . ...

... Dark Energy (Part of the Hubble Discoveries Series): http://hubblesite.org/hubble_discoveries/dark_energy/ (Flash-based multimedia tutorial on the discovery and meaning of dark energy; includes information on the origin and fate of universe) . ... Cosmology Visualizations from the NASA Universe Forum: http://www.cfa.harvard.edu/seuforum/einstein/resources_visual.htm#featcos (A series of computer visualizations of the evolution and structure of the universe, available in a number of formats.) ...

... Science . ... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Evolution of the interstellar medium in galaxies from redshift 0 to 1.5 . ... Science Users Information . ... Observing with ESO Telescopes . ... Science Software . ... ESO-MIDAS . ... ESO Data . ... ESO Science Newsletter . ... The project is to use public HST NICMOS spectra to search for star formation in galaxies at high redshift and investigate their evolution. ... Return to list of thesis topics ...