... Unbiased surveies of star-forming regions; evolutionary processes in star formation; IMF; determination of evolutionary tracers . ... Light elements; mixing in stars . ... Spectroscopy of low-mass stars in SFRs/associations: cluster formation, triggered SF, SFHs, accretion properties . ... Influence of cooling e and magnetic field on the formation of primordial stars . ... This email address is being protected from spambots. You need JavaScript enabled to view it. ... 39 0552752 251 . ...

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• A homogeneous chemical analysis of the inner Galactic disk from the first data
• Arcetri Star-Formation Group Publications

... Field of interest: data analysis and interpretation of X-ray observations of BHC and NS systems, astrophysics of compact objects and related phenomena: X-ray , optical and radio observations , shocks and stellar winds, emission mechanism, the spectral and timing analysis of the X-ray emission from microquasars ( signature of accreting BH), atoll- and Z-sources ( signature of accreting NS), modeling of INTEGRAL images % . ...

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• Igor Antokhin

... The close proximity of the Magellanic Clouds allows us to probe the nature of these star forming regions at small spatial scales. ... We present the spatial analysis, via aperture/annulus photometry, of 16 Large Magellanic Cloud (LMC) and 16 Small Magellanic Cloud (SMC) H II region complexes using the Spitzer Space Telescope's IRAC (3.6, 4.5, 8 ЮМm) and MIPS (24, 70, 160 ЮМm) bands. ... The IRAC, MIPS, UV, and HЮБ spatial analysis are compared with the spatial analysis of the TIR. ...

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• NICMOS STScI Analysis Newsletter 25
• The Large Magellanic Cloud's Largest Molecular Cloud Complex: Spitzer Analysis
• Ultraviolet through Far-Infrared Spatially Resolved Analysis of the Recent Star

Molecular Lines in Star Formation Regions ­ the ALMA Challenge Paul Jones University of New South Wales Universidad de Chile 1 Molecular Lines in Star Formation Regions - Molecular lines trace the kinematics and chemistry (composition) of molecular clouds. ... The lines also trace physical conditions such as temperature and density, complementary to mm/sub-mm dust continuum data e.g. ATLASGAL and ALMA continuum. ... Simple molecules (eg. ... More complex molecules (eg. ...

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• The Local Volume HI Survey (LVHIS)
• ATNF Colloquium
• цЃngel R. LцЕpez-SцЎnchez Webpage

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Measured radial velocities for the primary (full symbols) and secondary (empty symbols), phased with the orbital period of 5.9051102 0.0000023 days. ... HD 98088 is a synchronised, double-lined spectroscopic binary system with a magnetic Ap primary component and an Am secondary component. ... The magnetic field in the primary is predominantly dipolar, with the positive pole oriented approximately towards the secondary. ...

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• C.S. Jeffery, Research Astronomer
• Armagh Observatory Preprint No. 306
• Homepage of Gavin Ramsay

. ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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• Formation of the Earth

... Observatory . Public . Science . ... Science Users Information Science Software jump to navigation jump to content . Science Users Information . Observing Facilities . La Silla Paranal Observatory . Paranal Facilities . ... Observing with ESO Telescopes . ... Publications with ESO Data . ... Large Programmes . ... ESO/GTC Programmes . ... Service Mode Guidelines . ... Science Data Products Forum . Science Archive Facility . ... ESO Science Newsletter . ... VODA . ...

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• ESO - bh99
• ESO - Research Area: PLANETS AND STAR FORMATION
• ESO - Research Area: STELLAR STRUCTURE AND EVOLUTION

... Interstellar matter (Diffuse Interstellar Bands), Astrospectroscopy, chemical composition of stars, model atmosphere method, variable stars. ... Klochkova V.G., Galazutdinov G.A. "The spectra of blue stars in the globular clusters" Preprint SAO N71 1991 . ... Galazutdinov G.A., Krelowski J., Musaev F.A., Bikmaev I.F., "On the relation between the carriers of diffuse interstellar bands and the simple molecular species", MNRAS, 1997, V.292, P.414-418 < Download gziped PostScript file . ...

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• Access via e-mail

. Documents latest versions (PS and Latex)

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• The AstroStat Slog Blog Archive DOE Petascale Data Analysis Program
• Special Session on AstroStatistics at HEAD 2013
• The AstroStat Slog funding

... Accurate identification of physical binary star systems has become of increasing interest in recent years. ... Identification of physical binary star systems, with an estimated reliability of such identifications based on the theory of probability, is also important for current and future efforts to find binary star systems that are candidates for observations with the aim of determining their orbits and component masses. ... probability of the proximity of proper motions and ; . ...

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• ADASS Conference Series
• The EINSTEIN On-Line Service
• Statistical Consulting Center for Astronomy

... OOF . ALMA . ... OOF Index . Zernike Polys . GBT example . ... Observed data and analysis . The observed beam maps are shown in the first row of the table below. ... We show the best-fitting aperture and the best-fitting beams as the number of Zernike orders used for the fitting is increased. A sample OOF observed data set (top row) and the results of analysis with increasing number of Zernike polynomials used to parameterise the aperture. ... In-focus beam . ... Observed beams . ...

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• Astrophysics Group members - M Hobson
• Emily Curtis
• A 215 to 265 GHz spectral line survey of the Sgr B2 molecular cloud

Next: Cyg X-1 as a Up: Black Holes in Binaries Previous: Black Hole Creation in . The discovery of binary radiopulsars with massive unseen companions ( >3- ) would be of great importance to fundamental physics and modern theory of stellar evolution, providing a compelling evidence for the existence of BH in nature. The formation of binaries consisting of a BH in a pair with a radiopulsar (PSR) has been discussed previously by Narayan et al. ... Здесь должна быть Table 11 (Note к Table 11) . ...

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• The Model
• Parameters of the starburst
• Calculation of binary NS coalescence rates

... Aloisi, A. The Old Stellar Population . Alonso-Herrero, A. HST /NICMOS Observations of the . ... Balcells, M. HST-NICMOS Observations of Galactic . ... Baum, S.A. Investigating the Evolution of . ... Becklin, E.E. A Coronagraphic Search for . ... Clampin, M. The Old Stellar Population . ... Close, L. HST NICMOS Observations of . ... The Stellar Population in . Geballe, T.R. HST NICMOS Observations of . ... Greggio, L. The Old Stellar Population . ... Leitherer, C. The Old Stellar Population . ...

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• ADASS '97 Program Information
• A Color Analysis of NICMOS Parallel Observations
• The Formation and Evolution of LMC Rich Star Clusters: NGC 1818

. Home . Watchouts . Software requirements . Installation . Download . Documentation . Calibration . Help . The status of the SAS data reduction and analysis is now available as Appendix of the Science Validation reports. Matteo Guainazzi Inputs from C.Erd, F.Jansen, J.Osborne, S.Rosen, G.Vacanti, and M.Watson are gratefully acknowledged. Pages maintained by SAS librarian . Any question about SAS should be addressed to the XMM-Newton help desk . Updated on: November 18, 2006

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• XMM-Newton Science Analysis System: Main Page
• Dataset structure
• Description

... Project page . ... Project workpage . Turbulence in the Multiphase Interstellar Medium . Project I | ... Project highlight | ... Towards simulating turbulence with adaptive meshes . ... A. Kritsuk, P. Padoan, M. Norman . ... A. Kritsuk M. Norman . ... A. Kritsuk, M. Norman, P. Padoan . astro-ph/0411626 | ... P. Padoan, A. Kritsuk, M. Norman, A. Nordlund . ... Introducing Enzo, an AMR Cosmology Application . B. O'Shea, G. Bryan, J. Bordner, M. Norman, T. Abel, R. Harkness, A. Kritsuk . ...

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• Database of Optical Properties -- Level: subsubpage

. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Ionosphere and radiowave propagation: structure . The main page . Information . Publications: . 2011 - 2015 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2000 - 2004 . 1995 - 1999 . Participation in International symposiums and conferences: . 2013 - 2015 . 2011 - 2012 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2002 - 2004 . N.V. Pushkov . 09/04/2016 23:52 MSK . webmaster@izmiran.ru .

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... How How do molecular clouds collapse to form do very young stars evolve? do planets grow in circumstellar disks? ... Real-time protoplanetary/protostellar disk evolution - movies of disks in formation High sensitivity, 2 AU resolution cm-wave observations (100K, 0.2 mas, 8 GHz bandwidth, A/T 10,000) proper motions (Reid ­ Bryden et al 1999) dynamical timescales months-years How do very young stars evolve ? cm-waves probe inner few AU of accretion ...

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• http://www.naic.edu/vscience/schedule/tpfiles/WaldroptagT2042tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/WaldroptagT2042tp.pdf
• http://www.naic.edu/~astro/hiconference/hiconf_pdfs/aohi08_rosenberg.pdf

The evolution of galaxies is driven by the intricate power play between magnetically driven turbulence and the mass and gravity of its comprising gas and dust, a system which governs the formation of stars in the dense cores of the interstellar medium s giant molecular clouds. ... This results in separate relations for the star formation rate depending on the Mach number of the medium, differing from each other by up to an order of magnitude. ...

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• CHIAKI's Research
• COALA - Computational Astrophysics Laboratory
• Bruce A. Peterson -- Signature

... Адрес: Москва, 119002, Большой Власьевский переулок, дом 11 . ... 499)?241?0500, 241?1237, 241?4086 . ... Пройти под арочкой выхода из метро, повернуть налево и перейти бульвар (осторожно ? машины!), идти по Гагаринскому переулку до его пересечения с Большим Власьевским переулком (примерно минут 5?7, ориентир ? церковь за забором), где повернуть направо, пройти по Большому Власьевскому около 100 метров, слева в глубине двора (за сквериком) будет 4-этажное желто-зеленое здание ? ...

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• Semiclassical Microlocal Analysis (Fall 2003)
• Addresses (in Russian)
• Poncelet: workshop on Geometric analysis