... 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. ...

It is a matter of common knowledge that in processes of genesis and evolution of many solar phenomena participate magnetic fields of sunspots. ... As a basis for formation of the database we take data on magnetic fields, collected by set of observatories during many years of observations. ... Section "Magnetic field data" contains data of magnetic field observation for separate sunspots, presented in standard text format (ASCII). ... Description of structure of these files is presented here . ...

Chiaki Kobayashi, Ralph Sutherland How galaxies did form and evolution? - to answer this unsolved problem, we are simulating the formation and evolutionary history of galaxies in the Universe, including star formation, supernovae feedback, and chemical enrichment. Comparing the spacial distribution of elements within galaxies with observations, we will examine fundamental physical processes that drive galaxy formation. ... COALA : Universe Galaxy AGN Star Planet ...

The On-The-Fly Calibration (OTFC) system, publicly released in Dec. 1999, calibrated data at the time a user requested data from the archive. ... The On-The-Fly Reprocessing (OTFR) system replaced OTFC on May 16, 2001. ... UCHCOORD and OTFR. ... To address this issue, a new header keyword, PROCTIME, has been added to OTFR data to record when the system processed the data. ... OTFC . OTFR . ... POD file (original telemetry file) is retrieved from HST archive and passed to OTFR system. ...

... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...

... For a certain group of XMM PPS products (e.g. EPIC background maps, EPIC maximum-likelihood source lists, EPIC images, EPIC sensitivity maps) a list of commands is executed stored in an ascii file (hereafter check file). ... The tests include existence and parameter range checks for header key words and source tables columns of EPIC PPS Fits files. ... This check file performs existence and parameter range checks for EPIC PN, MOS1, MOS2 background maps in the energy bands 0,1,2,3,4 and 5. ...

... Next . comedi_do_insnlist -- perform multiple instructions . ... The function comedi_do_insnlist() performs multiple Comedi instructions as part of one system call. In addition, Comedi attempts to perform the instructions atomically, that is, on standard Linux kernels, no process preemption should occur during the instructions. ... This function can be used to avoid the overhead of multiple system calls, or to ensure that multiple instructions occur without significant delay between them. ...

The Wideband Arecibo Pulsar Processor - File Format Page . WAPP files have three sections that appear sequentially in this order: an ASCII header description, the binary header, and finally the actual binary data. ... The WAPP realtime observation engine does not produce files larger that 2 Gbytes. At one time this represented a fundamental limit to Linux files. ... Each file will have it's own header, even when the files are simply continuations of a single observation. ... long int . ...

... casa::LineCollapser< T, U > . ... Can the process function in the derived class handle a null mask? If not, LatticeApply ensures that it'll always pass a filled mask vector, even if the lattice does not have a mask (in that case that mask contains all True values). virtual void . process (U &result, Bool &resultMask, const Vector < T > &line, const Vector < Bool > &mask, const IPosition &pos)=0 . ... The class is Doubly templated. ... virtual casa::LineCollapser < T, U >::~ LineCollapser . ...

... Science . ... Science Users Information > Science and Technical Meetings > Conferences 2011 > Very Low Mass Stars and Brown Dwarfs . ... Observing Facilities . ... Observing with ESO Telescopes . ... ESO Data . ... This workshop will review the current progress in our understanding of low mass star and brown dwarf formation in nearby molecular clouds, and will bring together observers and theoreticians to promote an energizing discussion. ... Surveys for young very low mass stars and brown dwarfs . ...

... Classes . ... TelescopeTCP Class Reference . This TelescopeClient class can controll a telescope by communicating to a server process ("telescope server") via the "Stellarium telescope control protocol" over TCP/IP. ... TelescopeTCP (const QString &name, const QString &params, Equinox eq=EquinoxJ2000) . ... getInfoString (const StelCore *core, const InfoStringGroup &flags) const . ... getEquinoxEquatorialPos (const StelCore *core) const . ... getJ2000GalacticPos (const StelCore *core) const . ...

Semiconductor Home > Products > Mixed Signal and Analog > CCD IMAGERS Family > . SN761210, VIDEO-PROCESSING CIRCUIT . Device Status: Active . ... The SN761210 is a bipolar integrated circuit designed as a video processor for Texas Instruments CCD image sensors. ... During storage or handling, the device leads should be shorted together or the device should beplaced in conductive foam. ... Gain Control . ... Iris Control . ... Orderable Device . ...

Upload Information Template for Hobbes.nmsu.edu =============================================== Archive Name: top212.zip Short Description: VIO application to monitor CPU usage by process Long Description: VIO application to monitor CPU usage by process. ... The process list can be sorted according to various criteria (including CPU percentage, name, threads), and any process from the list can be selected to be killed. ...

. My astronomical research interests center on galaxy structure and evolution. Current topics include: . Polar-ring and interacting galaxies (see also new catalogue ) . Galaxy warps: statistics, properties and origin . Spiral galaxies at z~1: radial and vertical structure of stellar disks, statistics of interactions . Surface photometry and kinematics, dynamical modeling . Observational cosmology . Joomla Counter since Sep 1997

... The acquisition data base of meteorological temporal data including systematic and chronologic cataloque for Global Tropical Cyclogenesis (on the whole of World Ocean's aquatorium) for 1983-1992 time interval is developed and based on personal computer IBM PC/AT. ... The data base consists of the following units: 1. ... This data base offers a unique opportunity to analyze macro- and synoptic-scale temporal features of global tropical cyclogenesis as indivisible physical process. ...

PROS is a multi-mission x-ray analysis software system designed to run under the Image Reduction and Analysis Facility (IRAF). The analysis of x-ray data differs from that of other wavelengths due to the nature of x-ray data. ... Programs in PROS are called tasks. Tasks are grouped by function into packages. ... The qpspec task allows users to extract a background corrected spectrum from a QPOE file for use in PROS or for export to other analysis systems. model specification and fitting . ...

Most radio and modem clocks used for a primary (stratum-1) NTP server utilize serial ports operating at speeds of 9600 baud or greater. ... In order to reduce these errors, a set of special line disciplines and stream modules can be configured in the Unix kernel. ... Note that not all Unix kernels support line disciplines and of those that do, not all support System V streams. ... There are two line disciplines and a special streams module included in the distribution. ...

Next: Study to Install an Information System at the University of the Istanbul Astronomy and Space Sciences Department . ... NOAO 1 , P.O. Box 26732, Tucson, AZ 85726 . A system for publishing frequently updated information to the World Wide Web will be described. Many documents now hosted by the NOAO Web server require timely posting and frequent updates, but need only minor changes in markup or are in a standard format requiring only conversion to HTML. ... NOAO 1 . ...

ANTHONY LASENBY - COSMIC MICROWAVE BACKGROUND . The Cosmic Microwave Background (CMB) provides some of our best and most accurate information about the universe and its evolution. I have been involved in CMB research since 1978, and have worked on experiments including Tenerife, CAT, the VSA and most recently Planck and QUIJOTE . ... In addition, I am interested in several theoretical topics in CMB and early universe research. Planck at Launch . ... Cosmic Microwave Background . ...

... Figure: Massive binary evolutionary track. ... A short glance to this track is sufficient to understand that there are a lot of evolutionary scenario parameters, which affect different stages of the binary evolution. Fortunately, a very limited number of parameters has effect on the compact binary merging rate. ... The most important (and practically unique) parameter changing the galactic binary NS merging rate is the distribution of an additional (kick) velocity imparted to NS at birth. ...