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1. Analysis of (radio) spectra Bojan Nikolic web pages (r. 329)
... Bojan Nikolic web pages (r. 329) . ... The is the main page for code for Bayesian analysis of radio spectra and similar observational data. ... Nested Sampling in R & analysis of spectra . ... Paper I: Method . ... Observed radio spectra often consist of few measurements (typically 3?10) with significant errors against which it is tempting to try to fit a number of different models. ... page. ... Analysis of (radio) spectra . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/galevol/speca/index.html -- 11.3 Кб -- 04.04.2016
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2. ADASS 2002 Conference Proceedings
... CB3 0HA, U.K. The UCDs (Unified Content Descriptors) were first developed in the ESO/CDS data mining project, to describe precisely the contents of the individual fields (columns) of tables available from a data center. ... We present different applications of UCDs: selection of catalogues, based on their content; identification of catalogues having similar fields; automated data conversion allowing direct comparison of data in cross-identifications. ... a definition of the corresponding UCD; . ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass02/P1-1/ -- 12.7 Кб -- 12.03.2003
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3. Open Systems Handbook: A Guide to Building Open Systems
Open Systems Handbook: A Guide to Building Open Systems . ... This book is designed to provide interested individuals and organizations with an overview of open systems and the work being done to achieve them. ... This section is organized using a descriptive model of an open systems environment developed by the IEEE PI 003.0 Working Group, which is developing the Guide to POSIX-based Open System Architecture. ... Standards for open systems 13 . Chapter 3: The open systems environment (OSE) 15 . ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/rus/casr/os/3_12/1/13.htm -- 22.3 Кб -- 21.03.2016
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4. ESO - Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies
... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies using ALMA calibrator observations . ... ALMA . ... ESO-MIDAS . ... It is therefore essential to probe the evolution of cold gas over cosmic time. ... We are looking for an enthusiastic PhD student who is interested in working with us in using ALMACAL to address exciting and topical science questions related to the evolution of molecular gas in galaxies. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/activities/thesis-topics/abstr-zwaan1.html -- 29.5 Кб -- 10.04.2016
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5. Starburst and Galaxy Evolution Introduction
Stars are the fundamental building blocks of galaxies. ... Comparison between observations and models of evolving stellar populations helps understand the star formation process, triggering mechanisms, influence of the environment, the chemical history, and processes in the interstellar gas. Our research concentrates on galaxies with active current star formation. Many of these objects show signatures of violent high-mass star formation, a phenomenon often called `starburst'. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/starburst/intro.html -- 3.9 Кб -- 30.09.2008
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6. Late Stages of Stellar Evolution
... 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. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/plintel/groups/lsse/LsseHomePage.html -- 52.2 Кб -- 28.02.2014
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7. Astronomy HyperText Book: Stellar Evolution
... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, t