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1. Stars with Less Secure Periods
Next: Stars without Periods Up: Other Stars Previous: Stars with Highly . ... However, due to lower signal to noise their periods are less secure. ... This could be interpreted as a continuous distribution with statistically insignificant deviations which give the appearance of gaps or a real gap. ... When the distributions of periods greater five days are compared for the ONC stars and those near Orionis the KS test gives a 47% probability of these distributions being drawn from the same population. ...
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Ссылки http://hea-www.harvard.edu/~swolk/thesis/results/node6.html -- 8.3 Кб -- 02.10.2012
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2. HISA Poster for the 195th Meeting of the AAS, January, 2000
A press release on the Canadian Galactic Plane Survey was associated with this poster. ... Below are maps of HI emission, HISA, and 12 CO emission in the eastern 25% of the survey, given as projections along the velocity ( Figure 1 ) and latitude ( Figure 2 ) axes. ... 2000, A. J. , submitted . ... GIF | ... We are developing automated methods of locating HISA in velocity cubes by removing large-scale emission in space and velocity and flagging small-scale dark residuals. ...
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Ссылки http://www.naic.edu/~gibson/hisa/poster/2000/ -- 11.2 Кб -- 20.11.2005
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3. Results
... 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. ...
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Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/nisensonp.dir/section3_3.html -- 7.5 Кб -- 16.04.1994
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4. http://selena.sai.msu.ru/Shev/Publications/m44_76_sinitsin_shevchenko.pdf
FEATURES OF THE HYDROGEN DISTRIBUTION AROUND LUNAR CRATERS PROCLUS AND KEPLER. ... In result of analysis of the data Lawrence and Feldman constructed the hydrogen distribution on the lunar surface [1]. ... However, the authors shown, that EN flux data features may be explained by other element abundance in the lunar soils, namely: Si, Ca, Gadolinium (Gd), Samarium (Sm) and Fe. ... Using of the Feldman's interpretation of the Lunar Prospector data [8], we constructed hydrogen distribution map (Fig.1). ...
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Ссылки http://selena.sai.msu.ru/Shev/Publications/m44_76_sinitsin_shevchenko.pdf -- 164.0 Кб -- 16.03.2011
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5. Unified Radio Catalog: results for Version 1.1
... Radio Catalog . The corrections in NVSS fluxes leading to the corrected Version 1.1 also result in changes to some of the figures and tables in Kimball Ivezi? ... The results are qualitatively the same. ... The new versions of the figures, along with the original versions (in high resolution), are available here . ... These figures, along with Table 4, continue to motivate t = 0.35 as the optimal separator between "simple" and "complex" sources). ... Complex Sources . ... t NVSS . ... galaxy . ...
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Ссылки http://www.atnf.csiro.au/people/Amy.Kimball/version1.1_changes.shtml -- 8.3 Кб -- 27.02.2014
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6. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... While the traditional statistics of impact craters allow us to determine the cumulative meteoroid flux on the lunar surface, the recent successful identification of fresh craters in orbital imagery has the potential to directly measure the cratering rate of today. Time-resolved recordings, e.g., seismic data of impacts and impact flash detections clearly demonstrate variations of the impact flux during the lunar day. ...
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Ссылки http://star.arm.ac.uk/highlights/2012/629.html -- 6.6 Кб -- 18.12.2012
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7. APOD: December 26, 1997 - West Of The Great Red Spot
... December 26, 1997 . West Of The Great Red Spot . Credit: The Galileo Project , NASA . Explanation: The turbulent region West of Jupiter's Great Red Spot is highlighted in this recent picture constructed from data recorded by the Galileo spacecraft. The image is color coded to show cloud height and thickness ; white clouds are high and thick, light blue clouds are high and thin, and reddish clouds are low. ... About APOD > . ... NASA Technical Rep.: ...
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Ссылки http://www.sai.msu.su/apod/ap971226.html -- 4.2 Кб -- 02.10.2012
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8. http://www.mao.kiev.ua/lao/presentation/grytsai_Ozone%20and%20Strat%20Temp_Kiev%20SSch08.pdf
Variations of total ozone content and lower ozone stratosphere temperature in Antarctic Region during winter-spring period A.V. Grytsai National Taras Shevchenko University of Kyiv Astronomy and Space Physics Department assen@univ.kiev.ua Data, used in the work work Total ozone: Total Ozone Mapping Spectrometer (TOMS) measurements during 1979 - 2005 and Ozone Monitoring Instrument (OMI) ones for 2006, for http://toms.gsfc.nasa.gov/ftpdata.html. ... A long-term TOC decrease is significant. ...
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Ссылки http://www.mao.kiev.ua/lao/presentation/grytsai_Ozone%20and%20Strat%20Temp_Kiev%20SSch08.pdf -- 1659.8 Кб -- 24.09.2008
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9. Results scientific researchs LRS
Scientific results of the work of Laboratory of Radio Spectroscopy : . In presented messages outlined the results of scientific researches conducted by the stuft of LRS. ... Interaction of the Supernova Remnant S 147 with the Ambient Interstellar Gas . ... The spatial power spectra of galactic neutral hydrogen at high galactic latitudes . Properties of the interstellar gas clouds . ... Scaling relations and intrinsic motions in the interstellar neutral hydrogen clouds . ...
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Ссылки http://mavr.sao.ru/hq/lrs/result1.html -- 4.6 Кб -- 09.04.2016
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lrs/result1.html -- 4.6 Кб -- 09.04.2016
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lrs/result1.html -- 4.6 Кб -- 09.04.2016
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10. U of O High Energy Physics Seminars
... In this seminar, we will watch a recording of a seminar given at CERN on 23 September by Dario Autiero on behalf of the OPERA collaboration describing the results and the various technical effects which could contribute to the observed anomaly. 4:00pm, 412 Willamette Hall . ... Despite an initial CDF claim that the probability of this being an artifact of backgrounds was less than 1 part in 100,000, I will show how we went about demonstrating there is in fact no excess in the CDF Wjj data. ...
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Ссылки http://zebu.uoregon.edu/~uochep/seminars/seminars-fall11.html -- 3.8 Кб -- 09.01.2012
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11. http://xray.sai.msu.ru/~polar/html/publications/ring/shklovsk.ps
... 1 Figure 1: The density distribution in RZ plane Figure 2: The luminosity distribution in RZ plane for Maxwellian kick velocity (75 km/s) 2 Figure 3: The luminosity distribution in RZ plane for Maxwellian kick velocity (150 km/s) n(R; Z) = nHI + 2 \Delta nH2 nH2 = n 0 \Delta exp џ \GammaZ 2 2 \Delta (70pc) 2 – If 2kpc џ R џ 3:4kpc, then nHI = n 0 \Delta exp џ \GammaZ 2 2 \Delta (140pc \Delta R=2kpc) 2 – ; For R џ 2kpc n(R; Z) was assumed to be constant: n(R ! ...
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Ссылки http://xray.sai.msu.ru/~polar/html/publications/ring/shklovsk.ps -- 46.1 Кб -- 27.12.1997
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12. Is the incredibly slow rotation of Venus a result of a geologic cataclysm? |
... Tonight's Sky . ... SUN MOON MERCURY VENUS MARS, JUPITER SATURN . ... Venus . ... Sky this Month . ... Astronomy for Kids . ... Is the incredibly slow rotation of Venus a result of a geologic cataclysm? ... It appears unlikely that resurfacing, if it occurred, led to the slow rotation rate of Venus, but it certainly may have caused some changes to the speed. ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ...
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Ссылки http://www.astronomy.com/magazine/ask-astro/2012/03/slowpoke-planet -- 63.0 Кб -- 10.04.2016
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13. XWare > APOD
Astronomy Picture of the Day . Aurora Over a Communications Tower . ... Aurora light results from energetic electrons and protons striking molecules in the Earth's atmosphere. The Great Nebula in Orion . ... Fornax Cluster in Motion . ... Earths North Magnetic Pole . ... A magnetic compass does not point toward the true North Pole of the Earth. Rather, it more closely points toward the North Magnetic Pole of the Earth. The North Magnetic Pole is currently located in northern Canada. ...
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Ссылки http://www.astronet.ru/db/xware/apod.html?page=98&d=2007-05 -- 15.0 Кб -- 12.04.2016
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14. Redshift Distribution
... The distribution of redshifts among the DXRBS FSRQs identified so far (Figure 3) is quite similar to that of the 1 Jy and S4 samples. ... A more thorough comparison will have to await completion of our survey and the convolution of the redshift distribution with the WGACAT sky coverage. As has already been mentioned by Hook et al. (1996), selecting flat-spectrum sources is an efficient way of finding high-redshift, radio-loud quasars. ...
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Ссылки http://www.eso.org/~ppadovan/survey/dxrbs_paper/node12.html -- 6.5 Кб -- 03.12.2003
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15. Study of radio spectra and variability of GPS sources
... The results of long-term monitoring of Gigahertz-Peaked Spectrum sources were found the statistically significant differences (0.05 significance level) in the high-frequency spectral index distribution between subgroups of galaxies and quasars. ... This can mean that the electron energy distribution for GPS galaxies is steeper than for GPS quasars. ... The first area corresponds to GPS-quasars that have statistically larger value of redfhift, second area corresponds to GPS-galaxies. ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2011/Mingaliev/ -- 4.9 Кб -- 02.10.2012
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16. UHTC Coatings: Ultra High Transmission Coatings, Special Coatings, Telescopes,
... Telescopes ћ Binoculars ћ Microscopes . Meade Ultra-High Transmission coatings (UHTC ) Group . ... Meade Standard Coatings: The optical surfaces of all Meade telescopes include high-grade optical coatings fully consistent in quality with the precision of the optical surfaces themselves. ... These specialized, and extremely advantageous, coatings are offered here as the Meade Ultra-High Transmission Coatings (UHTC) group, a coatings group available optionally on many Meade telescope models. ...
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Ссылки http://www.meade.com/catalog/uhtc/index.html -- 24.8 Кб -- 10.11.2012
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17. Results and conclusions
Next: Bibliography Up: On the metallicities of Previous: Observations and data reduction . The results of chemical abundance determination for the studied galaxies are presented in Table 2 . The comparison of the respective data for UM 133 and UM 382 with the abundance ratios from Izotov & Thuan ([ 1999 ]) shows that they well agree with the derived average values for the sample of low metallicity BCGs. ... The full range of the velocity curve is about 100 km s -1 . ... UM 133 . ... UM 283 . ...
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Ссылки http://www.sao.ru/precise/Laboratory/Publications/2000/UM-reobs/node3.html -- 15.4 Кб -- 07.02.2000
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18. S.P. Korolev RSC Energia - International Space Station
... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... History . ... Educational reporting which elucidates the features of the space experiments conduct onboard the station (the ISS inertia tensor, etc.) and ways of the ISS attitude hold, on the attitude sensors and devices defining a space position of science devices, on deformation of the station hull, magnetic measurements, as well as microgravity disturbances onboard the station. ... 2015 JSC "S.P. Korolev RSC "Energia"...
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Ссылки http://www.energia.ru/en/iss/researches/popular/01.html -- 23.4 Кб -- 10.04.2016
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19. http://www.arcetri.astro.it/radtran/talks/cvlahakis.pdf
The SCUBA Local Universe Galaxy Survey Dust along the Hubble sequence Catherine Vlahakis University of Bonn Collaborators: Steve Eales (Cardiff University) Loretta Dunne (University of Nottingham) Overview What is SLUGS? Results from the survey Recent work using SLUGS results the FIR-radio relation Introduction: SLUGS SLUGS a submm survey of galaxies in the local Universe at 850m and 450m Survey of ~200 nearby galaxies: 104 60m-selected ("IRS") (Dunne et al. ...
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Ссылки http://www.arcetri.astro.it/radtran/talks/cvlahakis.pdf -- 460.3 Кб -- 25.06.2007
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20. http://astro.uni-altai.ru/AFgalleries.html
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Ссылки http://astro.uni-altai.ru/AFgalleries.html -- 1.1 Кб -- 01.10.2012
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