... 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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• WCSLIB: FITS-WCS and related software
• Related Programs
• The Local Volume HI Survey (LVHIS)

... Mindful of these biases, I can now explore the relations between the measured rotation periods and various other observables. The hypothesis behind monitoring stellar variability is that active stars have asymmetric spot distributions on their photospheres. ... They found that only stars with rotation periods greater than seven days show variations greater than 0.4 magnitudes at I. Bouvier et al . ... 1993a) demonstrated a relation between X--ray flux and spectral type in ZAMS stars. ...

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• List of Related Documents
• Statistics 310hfr 2004-2005
• The AstroStat Slog relations

... The (very) slow rotation of magnetic Ap stars. ... Magnetic stars in young clusters and associations. ... Magnetic fields in low-mass stars from high-resolution infrared spectroscopy. ... Magnetic field measurements of late B-type starss. ... Measurement of magnetic field of FK Com. ... Magnetic field of white dwarfs. ... The magnetic star evolution project (teleconference). ... Conference-2014 . Program . ... Laboratory for the Stellar Magnetism Study of SAO of RAS . ...

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• Publications

A Test of Galaxy Evolutionary Models Via Angular Sizes M. Im S. Casertano, R. E. Griffiths, & K. U. Ratnatunga (The Johns Hopkins University) The relationship between angular size, magnitude, and redshift of faint galaxies is explored as a potential tool to distinguish between different galaxy evolutionary models. ... The mild lumi­ nosity evolution model predicts more luminous galaxies of large angular size at high redshift, as does a standard no evolution model. ... 25) with redshift higher than z ? ...

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• The Mass Loss Return from Evolved Stars to the Large Magellanic Cloud:
• The State of the Gas and the Relation between Gas and Star Formation at Low
• Institute for Planets and Life

A comparative study of type I and type II supernovae . ... Sternberg State Astronomical Institute, Moscow, U.S.S.R. (Received 26 November, 1985) . ... No significant difference between SNe I and SNe II has been found in their radial distribution and frequency of outbursts in spiral galaxies. ... The radial distribution of type Ia SNe in spiral galaxies is only slightly steeper than the one for SNe II, while SNe Ib/c are more concentrated towards the central regions. ...

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• Gimp related links collection
• Zen: relation featur?s
• Music related links

International Service of Geomagnetic Indices (ISGI) of the IAGA . ... World Data Center C1 for Geomagnetism (WDC-C1), . Solar-Terrestrial Physics Division in Copenhagen, Denmark . ... Sodankyl Geophysical Observatory Geomagnetic and Ionospheric Data . Space Physics Text Book (Oulu): Magnetic activity indices . ... Solar Data Analysis Center (SDAC) . ... Mauna Loa Solar Observatory Analysis Center of HAO/NCAR in Boulder, Colorado . ... Neutron Monitor Server , University of Chicago . ...

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• Basic definitions [Oulu]
• Dispersion relation [Oulu]
• Geomagnetic Indices Kp, ap, Ap, Cp and C9

Next: EVOLUTION MODELS Up: EXTREME HELIUM STARS: PULSATION Previous: EXTREME HELIUM STARS . The characteristic surface properties, effective temperature , surface gravity and composition , of EHes have been summarized by Jeffery (1996). ... Helium: ( ) By definition, helium dominates the atmospheric abundances. ... This is supported by a correlation between N and Fe abundances in EHes. ... Next: EVOLUTION MODELS Up: EXTREME HELIUM STARS: PULSATION Previous: EXTREME HELIUM STARS Simon Jeffery . ...

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• Stars Beyond Maturity
• MASSES
• M.D. Smith, Research Astronomer

. Cambridge > Cavendish Lab > MRAO . Home . OOF . ALMA . IR . GalEvol . Lecturing . Home . Index . Publications list . Links . GPG key . Postal address . Interacting galaxies . Technical notes . OOF . OOF Index . Zernike Polys . GBT example . Why defocus? . OOF software . ALMA . Memos . Atmo . Pages related to publications . Clemens et al 2008, The history of star formation and mass assembly in early-type galaxies . Copyright 2008 Bojan Nikolic . Send feedback about the website to: b.nikolic@mrao.cam.ac.uk

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• Astrophysics Group Highlights & News
• Lectures and related materials
• ALMA related pages

... The evolution of a binary system can be described as the movement of a point in the parameter space , constituting both physical quantities (such as masses of binary components, their radii, luminosities, orbital period, etc., independently of direct observational measurability of these values Each binary traces a path (which we will call a ``track'') in this space, in a way strictly determined by the evolutionary scenario. ... Then the fraction of binaries lying inside is expressed by . ...

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• Conclusions
• Evolution of Magnetic Rotators in Non-circular Orbits
• Effect of sources evolution on

... From the uvby photometry and proper motions for about 5500 nearby F stars we have found the following: (i) F stars , taken in narrow ranges of metallicity , show at [fe/H] 0 rather distinct cut-off in their distribution along the Main Sequence (MS) at the blue side, which is suggested to be an indication for the MS turn-off in stellar groups of fixed metallicity ; (ii) the corresponding turn-off age from theoretical isohrones strongly correlates with the ...

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• Vladimir Marsakov Publication List
• RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures
• Subsystems of the Galactic halo, figures

PEGASE: Project de'Etude des Galaxies par Synthese Evolutive (by Damien Le Borgne and Brigitte Rocca-Volmerange) . Galaxy colours (by Robin Stevens) . ... Images of radio galaxies and quasars mapped at VLA . Atlas of radio galaxies in 3CRR sample (images, description, classification, etc.) Radio Galaxy and Quasar Images at Other Sites by A.Bridle . ... Radio galaxies in Abell clusters . ... Digitized Sky Survey images . Faint Images of Radio Survey at Twenty-cm at VLA . ...

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• Informational system "Evolution of RG"

по текстам по форуму внутри темы . Астронет | ... Форумы >> Обсуждение публикаций Астронета . ... Международная конференция "Putting A Stars into Context: Evolution, Environment, and Related Stars" . ... Международный научный оргкомитет, Государственный астрономический институт им. П.К. Штернберга, Институт астрономии РАН и Астрономическое общество проводят конференцию "Putting A Stars into Context: Evolution, Environment, and Related Stars" 3-7 июня 2013 г. в Москве в МГУ им. М.В. Ломоносова. ...

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• Астронет > Форумы > Обсуждение публикаций Астронета > Re: Международная
• Астронет > Поздние стадии эволюции звезд. Конспект лекций

... A universal physical relation for quasars . ... Harvey Tananbaum and his collaborators have first observed a relation between the soft X-ray and the optical/ultraviolet emission in AGN in 1979. Such relation is nonlinear, and it is usually parameterized as dependence between the logarithm of the monochromatic luminosities at 2500 †Е ( L 2500†Е ) and 2 keV ( L 2keV ) . ... Yet, the dispersion along the L 2500†Е тАУ L 2keV relationship is found to be rather high, typically ~0.35тАУ0.4 in log units. ...

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• Arcetri Solar Physics Group: Solar Polarimetry
• Arcetri Spectral Code related publications
• CHIANTI related publications

Do LIRGs follow the Tully-Fisher relation? ... For a small we can say majority of investigate i Conclusion number of galaxies in our sample, that the T-F relation holds. ... The purpose of this research was to study the LIRGs (Luminous Infrared Galaxies) and see if they follow the Tully-Fisher relation. The LIRGs are different to normal galaxies in the fact that they emit 90% of their light in infrared. ... The faster the galaxy rotates, the wider is the emission line in velocity. ...

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• E-ALFA at IAU Symposium 244
• The Evolution of Galaxies Seen Through The Neutral Hydrogen Line The Evolution
• Common Holidays in Relation to Equinoxes, Solstices Cross-Quarter Days

... Recent Topics . ... MAO main . ... The third-order space-by-time relation . ... Тема: The third-order space-by-time relation . ... The mass m experiences a gravity force toward the sun and . ... will experience the Coriolis force or Coriolis acceleration. ... differentiated space-by-time twice and discovered equation2. ... If one differentiates . ... time differentiation of space-by-time. ... third-order space-by-time relation. ... understand the third-order space-by-time relation. ... MAO NASU . ...

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• MAO NASU :: Topic: Fw: US-Russian Relations and the International Space Station
• КАРТОТЕКА ПУБЛ?КАЦ?Й СП?ВРОБ?ТНИК?В ГАО НАН УКРА?НИ

... Today, studies of resolved stellar populations constrain fundamental relations - such as the initial mass function of stars, the time scales of stellar evolution, the timing of mass loss and amount of energetic feedback, the color-magnitude relation and its dependency on age and metallicity - that represent key ingredients in our prescription to interpret light from the Universe and to measure the physical state of galaxies. ...

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• David Nicholls: CV and publications
• CHIAKI's Introduction
• CHIAKI's Research

Next: References Up: Multivariate Analysis Methods Previous: Correspondence Analysis . ... SHOW/TAB mytab . READ/TAB mytab . PRINT/TAB mytab . DELE/TAB mytab . ... To select group 2 members, defined in column 4, from table MYTAB; then plot coordinates defined in columns 1 and 2; then select group members; overlay the coordinates of these points on the initial plot with a different symbol; and finally to get a good quality hard--copy representation: . ... PLOT/TAB mytab . ...

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• The Echelle Relation
• Refining the Dispersion Relation
• Documentation: LEDA: parameter: mod0

Next: XEncirEn Up: CCF Components Previous: General CCF Components Contents . The mirror calibration files describe the X-ray response of the three XMM mirror modules. As a baseline, there will be one CCF constituent per telescope. ... Description . Generation from Ground Calibration Data . Generation from In-Orbit Data . ...

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• Housekeeping related keywords
• RGS Related CAL Routines
• Pattern related information

... 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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• The Tully Fisher Relation
• Astronomy Plus CCD Images of Galaxies
• Ozone Depletion

... The concepts of Fourier frequency and wavelet duration are obviously related. ... Among many sensible definitions, we chose to require that the peak of the wavelet mean spectrum should be matched with the singularity of the Fourier transform of the cosine wave. Then, it can be shown that the frequency of the cosine is related to the wavelet duration by the relation . ... The ambiguous definition of the duration of an event is common to the sizing of any object of irregular shape. ...

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• Historical Notes
• RELATED WORK
• Album: My woodworking and related stuff