Альтернативный форум . Scientific.ru Все форумы . ... Time (@) - 13.04.2007 09:15 . Re: Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results . x203a; x203a; x203a; в ответ на: Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results Котофеич . ... Re: Anisotropy in the Hubble constant as observed in the HST Extragalactic Distance Scale Key Project results Котофеич, 13.04.2007 13:37 . ...

. Update is coming soon.

... X 13- , - (W), 2.8 GHz (R2800), (SA), (FLA), (CorL), (ECH) (PCH) , (MSAS), (PF), (IMF), (CLI), (FSE) - (AA). , ( ) . ... E13, E5 ELM . ... ELM . ... 3 W R2800 SA FLA CorL ECH PCH MSAS PF IMF CLI FSE AA E13 E5 ELM rE rE -r E13 E5 ELM rE rE -r -0.43 0.48 0.88 -0.02 0.34 0.38 -0.10 -0.39 0.56 0.91 0.00 0.50 0.58 -0.12 -0.34 0.51 0.82 -0.02 0.22 0.38 0.53 -0.06 0.71 0.79 - 0.04 0.56 0.64 - 0.04 0.69 0.77 -0.08 0.34 0.39 -0.24 -0.22 0.52 0.63 - 0.04 -0.16 0.20 -0.27 0.40 0.42 +0.01 0...

Microsymposium 40, abstract 56, 2004 (A4 format) AUTOMATIC COMPILING OF HYPSOMETRIC MAP OF A PART OF THE 1 VENUSIAN SURFACE. ... The main principles applied in compiling the map such as the scale of the heights, types of prints and using of pictures of surface shall be apply in the compiling of the Hypsometric Map of Hemispheres of Venus in future. We consider that contours are the necessary features for hypsometric maps because allow to make measurement more accurate. ... Moscow., ...

... Uniformity of size and appearance of all the illustrations of the same type should be strictly observed. ... The numbers of curves, straight lines, etc., should be written in italics without any brackets both at an illustration and in text. ... In inscriptions, when the parameters of a curve are listed, the numbers of curves and notations of the parts of an illustration (a, b, etc.) should be placed in brackets prior to the corresponding parameters (a dash is not used). ...

... We thank the Swift team for their rapid scheduling of this observation. ... 2455705.20851 V 14.15 0.03 2455707.83079 V 14.10 0.03 2455710.84028 V 13.53 0.02 2455713.64631 V 13.66 0.02 2455714.65479 V 14.11 0.03 2455714.71823 V 14.12 0.02 2455714.78596 V 14.20 0.02 2455717.39593 V 14.37 0.03 2455726.62861 V 14.83 0.04 2455727.16343 V 14.57 0.04 2455730.50586 V 14.57 0.03 2455730.57329 V 14.56 0.03 2455730.70360 V 14.66 0.04 2455738.32865 V 14.00 0.02 2455742.86146 V 14.21 ...

. Cosmology . Very Early Universe . Cosmic Microwave Background Anisotropy . Dark Matter Models . Large Scale Structure . High Energy Astrophysics . Active Galactic Nuclei . Astrophysics of Compact Objects . Accretion Disks . Scientific Staff:

... How to Find Us . ... Take a stroll around the beautiful grounds of the Armagh Observatory Astropark. Armagh Observatory's Astropark is a scale model of the Universe where visitors can walk through the Solar System and into the Milky Way and beyond. The landscaped grounds are dotted with stainless steel scale models of the planets demonstrating how small our planet Earth is compared with some of its neighbouring worlds. ... Find out more about the Armagh Observatory Astropark. CONTACT US . ...

Lvov 2001 . Musical Kp diagram 2001 (*.pdf) . ... Horizontal intensity - H. Vertcal intensity - Z. from 0h. 00m. 1.01.2001 to 24h. 00m. 31.12.2001 . ... from 0h. 00m. 1.01.2001 to 24h. 00m. 31.08.2001 . ... from 0h. 00m. 1.01.2001 to 8h. 00m. 12.04.2001 . ... from 8h. 00m. 12.04.2001 to 8h. 45m. 25.05.2001 . ... from 8h. 45m. 25.05.2001 to 24h. 00m. 31.12.2001 . ... from 0h.00m.1.01.2001 to 24h.00Л.31.12.2001 . 0.50 min/mm . ...

O-C for observatory with code - 046. August , 2003 . ... 0.37 0.65 +/- 0.06 +/- 0.02 Internal error of single observation 0.12 0.04 ----------------------Compressed Ephemeris DE200/LE200 -------------- MP Obs Dynamical Time RA ( O-C )cosDEC DEC ( O-C ) h m s ' 65668 046 2003 8 27.963979 0 34 05.452 -0.33 +20 20 00.53 0.01 65668 046 2003 8 27.967079 0 34 05.376 -0.07 +20 20 01.42 0.07 65668 046 2003 8 27.967869 0 34 05.357 0.00 +20 20 01.62 0.05 65668 046 ...

Rastorguev А.S. "Astronomical Distances" (Lecture course for postgraduates, 2009-2016) . Part 1. ... Trigonometric parallaxes of stars. Moving clusters distances. ... Photometric distances: general approach. Normal stars as "standard candles". ... Main Sequence fitting or distance scale of star clusters. ... Moving photospheres technique. Cepheid distance scale and P-L relations. RR Lyrae distance scale. ... Globular clusters luminosity function. ...

MSU-E data examples. ... MSU-E . ... 16/03/1995 10:40 Msk . Pseudo-colour image. Red - channel 3, Green - channel 2, Blue -channel 1 . scale of projection 40 m/pixel . ... True-color image (786486K) . ... Channel 4 . ...

The multiscale analysis of heterogeneous structures is actually an important and effective tool of mathematical modeling in physics, technique and biology. ... The special year will extend the existing cooperation between French and Russian researchers in the multiscale analysis and in mathematical modeling in hemodynamics, taking into consideration the mass transport, coagulation, fluid-structure interaction and other aspects. ...

... I am involved in Project Astro, a program to bring astronomers into public schools to assist with teaching students about science and astronomy. ... While there are all sorts of scale model of the Solar System type exercises ( Mitchell Charity's page has a good listing of what's available), none were really tailored towards discovering the spatial relationships of the planets, and in a way that could be done at night as part of a Star Party. ...

... Seminar archive . ... Seminar archive 2011 3 June . ... Tristram K. D. A torus of molecular gas and dust is one of the key components of unified schemes of active galactic nuclei (AGN): it provides the material for accretion onto the supermassive black hole and is held responsible for the orientation-dependent obscuration of the central engine. I will present the results and current status of infrared interferometry of these dust distributions in AGN in the infrared. ... All seminars: . ...

. Lead Tungstate PbWO 4 . Application field . Scintillators . Structure . Tetragonal sheelite-type . Cleavage plane . (101) . Hardness (Moohs scale) . 3 . Growth method . Czochralski . Melting point . 1123 o C . Density: . 8.28 g/cm 3 . Wavelength of max. emission . 420-440 nm . Refractive index at emission maximum . 2.2 . Average decay time . 0.01 microsecond (gamma-rays, room temperature) . Max. crystal diameter . 50 mm . Cleaved PbWO 4 single crystal .

... mag . ... arcsec . ... deg . ... 2015-04-18 20:51:42 . ... Observation . ... Pulkovo . ... mag(j3+j1)-mag(j2) . ... Izmailov I.S. processed by . Izmailov I.S. ...

M87 Gas Disk and Optical Jet (STSci) . SEDS Messier Catalogue M87 Page (U. Arizona) . Black Hole and Jet in M87 (NASA/GSFC) . ... The large scale radio structure is shown in the 3CRR Atlas . Richard White's Virgo Cluster page has optical and X-ray images of the large-scale environment of M87 . ... HST Observes Distant Radio Galaxies (STScI) . HST Finds a Black Hole in NGC4261 (STScI) . HST finds a Bare Black Hole Pouring out Light in NGC6251 . ... Alan Bridle's Home Page . ...

. Comment on J1640+1220 . Augusto, Wilkinson & Browne (1998) show a 5 GHz MERLIN image and describe the source as a core-jet: their jet component is at PA=-50 . This, and our image, imply a gently curved jet from mas to 100 mas scale. The mas-scale structure is similar in the 8.4 GHz image from the VLBA Calibrators database. VLBApls home page . Last modified: 16 Oct 2000

0.17 0.16 0.15 0.14 +2 0.13 0.12 0.11 0.10 0.09 0 0 0 -1 +1 +s -2 -s 0.02 0.025 0.03 0.035 0.04 Coherent synchro-betatron mode tunes vs. the beam-beam parameter . Experiment and simulation 0.005 0.01 0.015