... Massive stars, having 10-150 masses of the Sun, with metallicities Z tens to hundreds times less than that of the Sun (Zo), are the main regulators of the galaxy formation and evolution processes in the early Universe. ... In this galaxy, using the 6 m BTA telescope, a new massive blue variable star with high luminosity (>=10 5 Sun's luminocities in visible light) was found. As far as its properties are concerned, this star falls into an LBV (Luminous Blue Variable) class of stars. ...

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• New LBV Star Discovered in the Galaxy
• Galaxy sector, archive 2010

Next: References Up: No Title Previous: Scientifically discovered God . What does it mean, God being discovered scientifically, or Superintelligence? And what is the future science dealing with an endlessly complicated world? ... But a human lexicon has also so important words as ``to understand'' and ``to believe''. ... And how the scientifically discovered God which has been inevitably reached by the modern simple science correlates with the religious God? ...

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• Scientifically discovered God
• No Title
• Evolution of the double neutron star merging rate and the cosmological origin

Welcome to the Starburst and Galaxy Evolution website.

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• HST this week: 092
• HST this week: 141
• Evolution of the HST Proposal...

... 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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• Formation and Evolution of Quasars

... Science . ... Science Users Information > Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Studying the Cosmological Evolution of Galaxy Clusters with (Sub-)mm Observations . ... Data Handling and Products . ... ESO Data . ... Studies of the Planck data set with optical and sub-mm follow-up observations give new insights about the early assembly of the first clusters, and the later evolution of their gas content as well as of their population of star-forming galaxies. ...

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• ESO - Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies
• ESO - Thesis Topic: Evolution of SN 1987A
• ESO - Thesis Topic: Evolution of Solar-type Stars using ALMA

... 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. ...

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• Local HI: Constraints on the evolution of the HI content of the Universe
• Radio Source Evolution Unified Schemes
• Programme - Abstract

Supernova 2009js in NGC 918 . This page is devoted to information on Supernova 2009js in NGC 918 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. Discovered independently by Lick Observatory Supernova Search (USA) and Koichi Itagaki (Japan). ... 2009/10/11.44 . 17.2 . ... Joseph Brimacombe . ...

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... AA(Max-Planck-Institut f r Radioastronomie, 53121 Bonn, Germany), AB(Max-Planck-Institut f r Radioastronomie, 53121 Bonn, Germany), AC(Max-Planck-Institut f r Radioastronomie, 53121 Bonn, Germany), AD(Special Astrophysical Observatory, Nizhnij Arkhyz, 357147, Russia), AE(Stockholm Observatory, 13336 Saltsj baden, Sweden) . ... 241B Structural and chemical changes during the AGB and post-AGB evolution are discussed with respect to two recent observational and theoretical findings. ... Abstract Text ....

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Family ASTRO was initially developed to expand the ASP?s flagship program Project ASTRO?, which has partnered thousands of volunteer amateur and professional astronomers around the country with classroom teachers and students in their communities. ... Since then, we?ve trained not only many Project ASTRO partners, but also hundreds of other educators across the country to use our series of Leader Kits and Take-Home Activities to lead fun, hands-on Astronomy Events in their communities. ...

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• ASP: Cosmology: The Origin, Evolution & Ultimate Fate of the Universe
• ASP: Responsible Exploration

Proposal Identification No.: P2472 Date Received: 2009-Feb-03 06:40:07 Technical Page Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Regular Pulsars 18 Hours 30 min. Phase-coherent timing of an LMXB-MSP transition ob ject We have discovered a bright nearby eclipsing millisecond pulsar with a non-degenerate companion, a key "missing link" in the evolution of low-mass X-ray binaries into radio millisecond pulsars. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/StairstagP2308tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/LazarustagP2722tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/SchomberttagA1369tp.ps

Next: EXTREME HELIUM STARS . EXTREME HELIUM STARS C.S. JEFFERY . ... Their exotic surface abundances point to previous evolution through the white dwarf sequence, followed by re-ignition due to a late helium shell flash or to a binary merger. ... I review the basic observational and theoretical properties of extreme helium star pulsations and show how these have been used to constrain evolutionary models, with particular reference to the cases of V652 Her and BX Cir. EXTREME HELIUM STARS . ...

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• PhD Thesis abstract
• Armagh Observatory Preprint No. 314
• CENTAURS: THE COMET-ASTEROID MISSING LINK

. SN 1997ef . NAME . UGC 4107 . DISCOVERED ON . Dec. 23 1997 . R.A. (2000.0) . 7h 57m . MAGNITUDE . 16.1 . DECL. (2000.0) . +49° 33' . TYPE . latest spectrum Ib . MAGNITUDE . OFF