. unfiltered . PC 1 - average . PC 2+3 - annual . PC 2 . PC 3 . PC 4 - secular . PC 5 . PC 6 . Sum of nine first PC's 1-10 . Difference between the initial signal and ten first PC 1-10 .

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Astrophysics graduate student programs . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... ATCA . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

... GBT results . ... OOF Holography Home Page Quick Links: . ... This page contains the more recent measurements with our new OOF Holography system. ... The latest Out-Of-Focus data were taken with SCUBA on 11th February 2003. ... Aperture . ... Residuals . ... The results are summarised in the following plots: ~~available soon - see previous results page for now~~ . We have recently obtained some OOF data from the Green Bank Telescope operated by the NRAO in the US. the results are shown here. ...

... 2014: . Suppression of cooling by strong magnetic fields in white dwarf stars . ... 69, 439, 2014. Evidence of supercritical accretion in SS433 . ... We discovered a flat portion (white noise) in the power spectrum of SS433 due to an abrupt increase of the disk thickness in the supercritical region. ... Both the hard X-ray radiation and the visual light are seen reflected from the walls of the funnel that forms in the wind of the supercritical disk of SS433. ... Archive . ...

... The results of Fabry-Perot interferometric study of XMD BCG HS 2236+1344 with two bright star-formation regions (probable merger). Upper row: Images in continuum and in H-alpha line in greyscale, with isophotes overlaid. Bottom row: the velocity field with the abrupt break, indicating the two components are probably unrelated (right); H-alpha line widths (FWHM) (or velocity dispersion) in km/s (also in greyscale and isolines) along the both components (left). ...

Find Similar Abstracts . ... The velocity of clusters of galaxies relative to the microwave background. ... BACKGROUND RADIATION, GALACTIC CLUSTERS, MICROWAVE SCATTERING, VELOCITY MEASUREMENT, HIGH TEMPERATURE GASES, MICROWAVES, POLARIZED RADIATION, RADIAL VELOCITY, RADIO ASTRONOMY, THOMSON SCATTERING . ... Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...

... We have been using it to analyze PC images of known gravitational lenses and QSOs which are candidates for lensing (Falco 1993). ... Fig. 1 plots the higher contours of the PC image of 0142 in the upper left, and its power spectrum in the upper right. ... If we fit the envelope of the power spectrum with a binary model, we find that best fit gives a separation of the two components of 1.3 PC pixels or about 58 mas. ... The lower two curves are cuts through the 0142 power spectrum. ...

... Science . ... Science Users Information > Science Publications > Science Announcements > Release of Photometric Catalogue Data Resulting from the VISTA Magellanic Survey . ... The catalogues were extracted from the reduced images which have been released under VMC Data Release 2 in June 2013. The new catalogue data are accessible from the ESO catalogue facility query interface , each accompanied by a comprehensive description; see for example, the description of the YJKs master catalogue. ...

Marc White . ... Turbulent entrainment processes may play an important role in the outflows from young stellar objects at all stages of their evolution. In particular, lateral entrainment of ambient material by high-velocity, well-collimated protostellar jets may be the cause of the multiple emission-line velocity components observed in the microjet-scale outflows driven by classical T Tauri stars. ... University of Amsterdam; STARPLAN, Copenhagen, Jul 2013 . ... E marc.white@anu.edu.au . ...

... Samara State Aerospace University Staff Timchenko Pavel Evgenevich . ... Raman spectroscopy. ... Timchenko E.V. , Timchenko P.E. , Taskina L.A. and others. ... Timchenko P.E. , Timchenko E.V. , Zherdeva L. A. and others. ... Timchenko E.V. , Timchenko P.E. , Shamina L.A. , Zherdeva L.A. Raman spectroscopy for the control of the atmospheric bioindicators // Remote Sensing and Modeling of Ecosystems for Sustainability XII, 11 - 12 August 2015, San Diego; United States, Publisher: SPIE, 2015, P. 1-8 . ...

... Equipment . ... The scientific-methodical work is an important component of the LSR work, which should satisfy the needs of employees of other laboratories of the ISSP RAS both in structure investigations and in interpretation of the obtained results. ... X-ray works: . ... the equipment for of X-ray topography: a spectrometer on the base of D4C source and the goniometer A-4 (Rigaku firm), a spectrometer on the base of RU-200 , the two-crystal spectrometer URT-2 (Russia), . ... LSR ISSP RAS . ...

... Recent Results . Publications . last 10 years in ADS) . ... This page is designed by A.V. Moiseev . ... The extended gas origin and kinematics in the fading AGN host galaxies" . talk on EWASS-2015, La Laguna, Jun 22-26, 2015) . Related publication: Keel et al. ... Related publication: Afanasiev V.L. et al. ... Related publication: Afanasiev V., Moiseev A. 2011, Baltic Astronomy, 20, 363 see in ADS . ... Related publication: Moiseev et al. 2011, MNRAS, 418, 244 see in ADS . ...

... Even future mission archives tend to concentrate more on what can be extracted out of a proposal or a Guaranteed Time Observation log than the actual extracted science out of the data itself. ... A year later the data is then publicly available. An archive researcher has then to go through a mass of data to find what may be useful without any indication as to what the actual observer's results were while using the data except the proposal, which in most cases is very general. ...

X­RAY STUDY OF CRAB­LIKE AND COMPOSITE SNRS K. TORII, H. TSUNEMI Osaka University AND P. SLANE Harvard­Smithsonian Center for Astrophysics 1. ... We have observed several objects including 3C58, CTA1, and G292.0+1.8. ... 1997; Torii et al. 1997). ... Al­ though the center­filled radio morphology suggested an interior plerionic component, strong X­ray emission lines seemed to rule out such specula­ tions. ... G292.0+1.8 0.5 ­ 2 keV G292.0+1.8 2 ­ 10 keV Figure 1. ASCA SIS images of G292.0+1.8. ...

. An example of ULF electromagnetic fields detection by the IESP-2M instrument. The figure presented is the dynamic spectrogram. E and B components are measured in satellite coordinates. Observations were made in the auroral region. Electromagnetic turbulence, which was observed mostly in electric components, is typical for this phenomenon. Fig.1 .

... Credit Copyright: ESA / Rosetta /MPS for OSIRIS Team ; MPS /UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA Explanation: Why does this comet's nucleus have two components? The surprising discovery that Comet 67P/ChuryumovGerasimenko has a double nucleus came late last week as ESA 's robotic interplanetary spacecraft Rosetta continued its approach toward the ancient comet's core. ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ... Comet 67P from Spacecraft Rosetta . ...

... Authors: Spyros Basilakos (Imperial College London) . ... Title: Populating a cluster of galaxies - I. Results at z=0 . ... Title: The Merger Rate to Redshift One from Kinematic Pairs: Caltech Faint Galaxy Redshift Survey XI . ... Title: Multi-wavelength observations of an evolved galaxy group: An endpoint of galaxy merging? ... 23 matches for the search pattern galaxy merging . The URL for this page is: http://xxx.itep.ru/find/astro-ph/1/galaxy+merging/0/1/0/past,all/0/0 www-admin@xxx.lanl.gov ...

... Last modified on August 19, 1996 by A. Richichi . ... Hamilton, D.P., Herbst, T.M., Richichi, A., B?hnhardt, H., Ortiz, J.L. 1995, '' Calar Alto observations of Shoemaker-Levy 9: characteristics of the H and L impacts '', Geophysical Research Letters, 22 , 2417. ... Hamilton, D. P., Herbst, T. M., B?hnhardt, H., Ortiz-Moreno, J. L., Richichi, A., Calamai, G. 1995, `` Calar Alto Observations of the A, H, L, Q1 and Q2 Impacts '', Proceedings of the XXIInd General Assembly of the IAU, den Haag 15-27...

... NED Home . ... Number of Essential Note) RA DEC Type km/s z Qual arcmin Refs Notes Phot Posn Vel/z Assoc Imag 8 30000 1.302000 .. 17 0 7 3 0 0 Retrieve 22 30000 1.469000 .. ... 51 6 14 2 0 0 Retrieve 131 30000 1.238000 .. ... 14 4 6 3 0 0 Retrieve 330 30000 1.760000 .. ... 15 2 6 3 0 0 Retrieve 552 30000 1.779000 .. ... 131 4 27 5 0 1 Retrieve 561 30000 1.500000 PHOT .. ... 143 5 36 5 0 0 Retrieve 572 30000 1.401000 .. ... 15 0 4 1 0 0 Retrieve 650 30000 1.760000 .. ... Back to NED Home ...

... In this first example, we allow an object to fall onto a small radar unit . The resulting Time-Frequency distribution is shown as a contour plot in Fig. 8 (a). Figure: FIGURE GOES SOMEWHERE IN THIS GENERAL VICINITY . ... Its density plot appears as an image in Fig. ... The response has a very high peak, as evidenced from Fig. ...