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... Tonight's Sky . ... Observing . ... Sky this Month . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... galaxies . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Open cluster NGC 2818, spiral galaxy NGC 2964, and spiral galaxy NGC 2976 . ... Astronomy for Kids . ... California Institute of Technology, Pasadena . ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

Peremennye Zvezdy", . ... Star Name: . GSC 4487-00399, . ... During observations of GSC 4487-00347, a new eclipsing binary star with an eccentric orbit (Otero et al. 2006), we discovered variability of GSC 4487-00399. ... We suggest that the star is a close-binary EW-type variable with the ephemeris: . ... Light Curve . The spectral window (1a), the power spectrum (1b), and the phase diagram (1c) of the variable star GSC 4487-00399. ... The finding chart for the variable star GSC 4487-00399. ...

Proceedings of the Particle Physics and Early Universe Conference (PPEUC). For this paper: postscript PPEUC CMB index 1 Likelihood Analysis.. ... Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, U.K. Max Tegmark . ... We discuss the problems of applying Maximum Likelihood methods to the CMB and how one can make it both efficient and optimal. ... A much fuller account of most of this work is available ( Tegmark, Taylor & Heavens (1997) ). ...

... Observations worldwide · 17 Haumea-Namaka events visible worldwide in 2009 · 18 telescopes of 2 m aperture on six continents observing as part of this international campaign · Five events visible from Australia in 2009 useful enough Simply combin global minimu the fit, going fr 1.10, althoug Adding the Ke the error bars a parameters. ... We recorded a comparison lightcurve of Haumea on the preceding night. This was necessary as Haumeas intrinsic lightcurve varies on timescales of ~1 week. ...

... В четверг, 14 апреля 2016 г., состоится семинар кафедры астрофизики. Повестка дня . ... Начало в 11 час.15 мин. Ауд. ... В четверг, 31 марта 2016 г., состоится семинар кафедры астрофизики . ... В четверг, 24 марта 2016 г. , состоится семинар кафедры. ... В четверг, 17 марта 2016 г. , состоится заседание кафедры. ... ОСП НИИ ПММ Национального исследовательского Томского государственного университета) . ... Copyright 2016 Астрономия в Санкт-Петербургском университете . ...

... ORGANIZATIONS: The Geological Society of America (Honorary Fellow); The American Geophysical Union (Fellow); The American Association for the Advancement of Science (Fellow); The American Institute of Aeronautics and Astronautics (Fellow); Sigma XI; American Association of Petroleum Geologists (Fellow); The American Institute of Mining, Metallurgical and Petroleum Engineers (Honorary Member); New Mexico Geological Society (Honorary Member); The American Astronautical Society. ...

VACUUM ARC DEPOSITED NANOSTRUCTURED TI COATINGS B.B. STRAUMAL1,2, N.F. VERSHININ1, E. RABKIN3, R. KROEGER3, R. DIMITRIOU4, and W. GUST2 1 I. V. T. Ltd. ... 92 - 70174 Stuttgart - Germany 4 3 Dpt Materials Engineering - TECHNION-Israel Institute of Technology - 32000 Haifa - Israel PECHINEY CRV - BP 27 - 38340 Voreppe - France ABSTRACT: Ti coatings on silicate glass substrates have been produced using a nonfiltered vacuum arc deposition technique. ... If the deposition time t is high, the Fig. ... Fig. ...

... IRAF supports two kinds of parameters, auto parameters and hidden parameters, which are treated differently. auto parameters are updated every time a task is run. ... Parameters for each task are contained in `parameter files' in the uparm sub-directory in `myiraf'. ... im > imhead.longheader=yes # explicitly setting <task.param>=<value> im > eparam imhead # Edit the parameter file to update one or more # parameters at the same time # see next section . ...

Next: Other parameters of the Up: The Model Previous: Initial binary parameters . As we only deal with initially massive binary systems (their primary's mass is higher than 10 ), which are capable of evolving off the main sequence during less than years, the compact stars left behind stellar evolution are (in the case of the most massive stars) NSs and BHs. ... For a NS belonging to a binary, the evolution complicates as the secondary star evolves: for example, (recycling), etc. ...

... Hubble Space Telescope Telemetry Access using the Vision 2000 Control Center System (CCS) M. Miebach European Space Agency, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland USA 21218 M. Dolensky Space Telescope ­ European Coordinating Facility, Karl­Schwarzschild­Str. ... Part of CCS is a Space Telescope Engineering Data Store, the design of which is based on modern Data Warehouse technology. ... A WEB­based user interface allows easy access to the archives. ...

Magnetic Flux of EUV Arcades and Dimmings as a Relevant Parameter . ... We study events of the 23th cycle, in which major non-recurrent geomagnetic storms (GMS) with Dst < - 100 nT are sufficiently reliably identified with their solar sources in the central part of the disk. ... Figure 3: FD magnitude vs. eruptive magnetic flux . Figure 4: Geomagnetic storm intensiry (Dst index) vs. eruptive magnetic flux . Figure 5: Geomagnetic storm onset and peak transit times vs. eruptive magnetic flux . ...

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