Next: Finding Young Pulsars Up: Young Energetic pulsars Previous: Young Energetic pulsars . ... Table 1: Young Energetic Radio Pulsars. ... Figure 20: The radio pulsar equivalent of the Hertzsprung-Russell diagram - a physical diagram indicating the nature and evolution of neutron stars. Each dot represents a pulsar, stars represent pulsars associated with supernova remnants, circles indicate pulsars in binary systems and ellipses indicate pulsars in binary systems with eccentric orbits. ...

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• Young Energetic pulsars
• Duchamp Source Finder
• User Parameters - Continuum Source-finding CentralProcessor 0.11 documentation

... Are HVCs a common feature of star forming galaxies? ... Consider the typical properties of the smallest HVCs (compact HVCs) found in HIPASS: . Distance . HI Mass . ... At 5 kpc . meager objects ~116 solar masses . ... 1.15 x 10 4 solar masses . ... Putman et al. (2003) found none to 10 7 solar masses. 2% of Sculptor to 3 x 10 6 solar masses by de Blok et al. (2001) found none. ... High velocity gas around other galaxies can be identified from maps and dynamics: . ... 2003) . ...

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• Pulsar Highlights - ALFA Finds Youngest Binary Pulsar Ever

... We show the analysis of low-hard and intermediate states of sources XTE J1550-564, H 1743-322, GX 339-4, XTE J1859-226, XTE J1650-500 and GRS 1915+105. ... Directly applying the scaling technique we also obtain that a ratio of the BH masses in XTE J1859-226 and in XTE J1550-564 is , and the corresponding ratio for XTE J1650-500 and XTE J1550-564 is . These values of scaling factors r implies that BH masses are ; solar masses in XTE J1859-226 and XTE J1650-500 respectively. ...

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... Translate Abstract . ... Structure and properties of IRC+10216 . ... AA(Stockholm Observatory, SE--133 36 Saltsj baden, Sweden), AB(Special Astrophysical Observatory, Nizhnij Arkhyz, Karachaevo-Cherkesia, 357147, Russia), AC(Max-Planck-Insitut f r Radioastronomie, Auf dem H gel 69, D--53121 Bonn, Germany), AD(Max-Planck-Insitut f r Radioastronomie, Auf dem H gel 69, D--53121 Bonn, Germany), AE(Max-Planck-Insitut f r Radioastronomie, Auf dem H gel 69, D--53121 Bonn, Germany) . ... Abstract Text . ...

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• Plug-and-Play-HOWTO : Tell the Driver the Configuration
• AGB and Post-AGB Evolution: Structural and Chemical Changes

Next: Arunav Kundu Up: STScI Science Jamboree Previous: Anuradha Koratkar . At the moment most of my time is spent studying the host galaxies of powerful AGN - quasars and radio galaxies - to try to find out how the properties of the host affect those of the active nucleus (and vice versa), and also how galaxy evolution is related to that of the AGN population. ... In pursuit of this I also do a lot of work on Seyfert galaxies and RQQs with the VLA and other radio telescopes. ... 3/24/1998 ...

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• Blind Deconvolution
• CSPICE Routines: DAFFPA_C
• Local astronomers find gigantic halo around neighboring galaxy - By MEGHA

... 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 ...

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• PPT Slide
• The history of star formation and mass assembly in early-type galaxies Bojan
• Galaxy Evolution Bojan Nikolic web pages (r. 329)

... 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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• Astronomy HyperText Book

... This thread illustrates a step-by-step recipe to perform EPIC sources detection. ... However, some users - in particular SAS novices - may find useful to perform each individual step of the source detection algorithm, to achieve a better control and understanding of its outcomes. ... The event list MOS.evt is assumed to have been already cleaned for high-background intervals, following, e.g. , steps 3. to 5. in the edetect_chain thread . ... An example of MOS background map is shown in Fig.3. ...

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• Example 8: Finding the cross-region ARF
• List of CAL Routines used

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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• Frequency of fading events
• EXTREME HELIUM STARS
• EVOLUTION MODELS

Find Similar Abstracts . ... The theory of large-scale structure of the universe - Local properties and global topology . Authors: . ... 00/1983 . ... ASTRONOMICAL MODELS, BIG BANG COSMOLOGY, GALACTIC CLUSTERS, GALACTIC STRUCTURE, UNIVERSE, ANISOTROPY, GALACTIC EVOLUTION, NEUTRINOS, TOPOLOGY . ... Use: Authors Title Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...

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• Why must a radiopulsar coupled with an optical star have high eccentricity?
• Introduction
• Ejector-propeller hysteresis

... 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; . ...

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• The XTE Data Finder (XDF)
• A New Entropy Measure Based on Multiple Resolution and Noise Modeling
• Spatial Structure of NGC 6822: An Example for Statistical Modeling of

Next: *imcnts* - Find counts Up: Regions and Source Parameters Previous: *isoreg* - A region . ... xi xspatial # Load the spatial package xs imcnts # Run the task to count photons source image file : xdata$rp110590.qp # Input file , use complete filename source region descriptor: c 6930 9390 240 # Circle at 6930 9390 # with radius of 240 pixels background image file or cts/pixel: xdata$rp110590.qp # From the same file bkgd region descripton: a 6930 ...

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• *imcnts* - Find counts in an extended region, after removing an embedded point
• Target Finding
• Where to Find Example/Test Code

Next: ANALYSE/ROMAFOT Up: The Interactive Path Previous: The Interactive Path . FIND/ROMAFOT frame [cat_tab] . This command works exactly like SELECT/ROMAFOT and therefore needs no detailed explanation. The only difference is that FIND/ROMAFOT , designed to select many stars, stores the positions of the objects in a catalogue table which has a different structure than then the intermediate table created by SELECT/ROMAFOT . This table serves as as input for the command ANALYSE/ROMAFOT . ...

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• About This Guide
• Version, UI, and Status Information
• Basic principles of time series analysis

Next: Examples of data contained Up: Electronic database Previous: Future plans . In astrophysics, the optical constants mainly are used to calculate the optical properties of scatterers, i.e. cross-sections, scattering matrix, etc. ... Optical properties derived from such models have been discussed in some books (see, e.g., [ 2 , 3 ]) and in principle can be calculated by using various light-scattering tools which are freely available via the internet [ 4 ]. ...

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• Hydrogenated amorphous carbon
• Extinction properties (transmitted radiation)
• Scattering properties

... We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. ... Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. ... The derived temperature maps are quite similar to the ones obtained earlier with a different methods, the main differences occurring in the spot latitudes and relative strength of the spot structures....

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... A Hidden object is used for passing name/value pairs when a form submits. ... JavaScript 1.0 . JavaScript 1.1: added type property The HTML INPUT tag, with "hidden" as the value of the TYPE attribute. ... Property . ... The form contains a "Display hidden value" button that the user can click to display the value of the Hidden object in an Alert dialog box. ... P><INPUT TYPE="button" VALUE="Display hidden value" NAME="button2" . ... Form name:<INPUT TYPE="hidden" NAME="h1" VALUE="Beluga"> . ...

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• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/packages.htm
• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/mimetype.htm
• About this Book

To find a single file below the current directory: find . name mtg_jan92 -print . This displays the pathname to the file mtg_jan92 starting from the current directory. ... To find a file below your home directory: find ~/ -name README -print . This displays the pathname to every file with the name README in your home directory or its subdirectories. ... name '*.fm' -print . This displays the pathname to any file with the extension .fm which exists below the current directory. ...

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• Editing a previous command line
• Examples of executing commands with the find command
• Finding a file

... Вход в Астротоп + Напомнить пароль + Блог + ЗАРЯ + Exit . ... Поиск сайтов в нашем каталоге (по части: адреса/названия/авторства): . ... Назад, на титульную страницу AstroTop-100 . ... Все замечания и предложения по поводу работы проекта AstroTop of Russia Вы можете оставить в гостевой книге . ... Вольф Александр , ему слать все замечания по идеологии и содержанию проекта. Программирование: Самодуров Владимир, Вольф Александр . ... Александр Вольф . ... AstroTop of Russia Гостевая книга . ...

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Next: Survey Methods Up: THE DEEP X-RAY RADIO Previous: THE DEEP X-RAY RADIO . Blazars are the most extreme variety of AGN known. ... The beaming hypothesis has been successful in reproducing the luminosity function of samples of blazars (e.g., Padovani & Urry 1990, 1991, 1992; Urry, Padovani & Stickel 1991), allowing the derivation of class properties such as the range of Lorentz factors and opening angles in the radio band (and also in other bands for BL Lacs). ...

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• Sample Properties
• Colours and magnitudes
• Previously Identified Sources

... 7.1 Introduction to media types . ... 7.3 Recognized media types . 7.3.1 Media groups One of the most important features of style sheets is that they specify how a document is to be presented on different media: on the screen, on paper, with a speech synthesizer, with a braille device, etc. Certain CSS properties are only designed for certain media (e.g., the 'cue-before' property for aural user agents). ... For example, the 'font-size' property is useful both for screen and print media. ...

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• Dynamic HTML in Communicator
• Visual effects
• Assigning property values, Cascading, and Inheritance