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http://www.stsci.edu/~marel/abstracts/abs_R31.html.
http://www.stsci.edu/~marel/abstracts/abs_R31.html.
1. VLA 404 compact sources
... Accurate positions of 404 compact radio sources used as calibrators by the VLA are presented. In addition, the structure and polarization of each source at both 4885 and 1465 MHz are given. ... Amplitude calibration was based on 3C286, whose fluxes at 4885 and 1465 MHz were assumed to be 7.41 and 14.41 Jy, respectively, in accord with the scale of Baars et al. (1977). short description of columns, as taken from the publication: . 1 source name . ... 8 Polarized flux at 4885 MHz (mJy) . ...
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Ссылки http://www.sao.ru/cats/doc/VLA404.html -- 4.5 Кб -- 18.03.2015
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2. Abstract
The Connection between Nuclear Structure, Central Black Holes and Radio Properties of Brightest Cluster Galaxies . ... 2001. ... We present preliminary results from an ongoing survey of nearby brightest cluster galaxies (BCGs), selected from the sample of Lauer Postman (1994). ... The profiles were fitted with generalized NUKER-law parameterization and an estimate for the central supermassive black hole mass was then obtained from adiabatic black hole growth model fits. ...
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Ссылки http://www.stsci.edu/~marel/abstracts/abs_A14.html -- 3.9 Кб -- 15.11.2001
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3. X-Ray Microlensing of Bright Quasars
... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Australia Telescope Online Archive (ATOA) . ... Parkes | ... Australia Telescope 20GHz Survey . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... X-Ray Microlensing of Bright Quasars . ...
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Ссылки http://www.atnf.csiro.au/pasa/18_2/mineshige/paper/index.html -- 50.9 Кб -- 08.04.2016
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4. Structure and properties of IRC+10216
... Translate Abstract . ... Structure and properties of IRC+10216 . ... AA(Stockholm Observatory, SE--133 36 Saltsj baden, Sweden), AB(Special Astrophysical Observatory, Nizhnij Arkhyz, Karachaevo-Cherkesia, 357147, Russia), AC(Max-Planck-Insitut f r Radioastronomie, Auf dem H gel 69, D--53121 Bonn, Germany), AD(Max-Planck-Insitut f r Radioastronomie, Auf dem H gel 69, D--53121 Bonn, Germany), AE(Max-Planck-Insitut f r Radioastronomie, Auf dem H gel 69, D--53121 Bonn, Germany) . ... Abstract Text . ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2001/mens_2001.html -- 12.1 Кб -- 28.12.2007
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2001/mens_2001.html -- 12.1 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2001/mens_2001.html -- 12.1 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2001/mens_2001.html -- 12.1 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2001/mens_2001.html -- 12.1 Кб -- 02.10.2012
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5. GSAOI Bulk Motions Science Page
... GSAOI Home . ... Science . ... It is widely accepted that the evolution of the large scale structure of the Universe is driven by dark matter. Understanding this dark matter continues to be one of Astronomy's great unsolved problems. Measuring the bulk motions of galaxies allows us to map the overall mass distribution of the Universe in a way that is independent of the luminous matter in galaxies. ...
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Ссылки http://www.mso.anu.edu.au/gsaoi/science/bulk.shtml -- 6.9 Кб -- 01.10.2012
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6. Шевченко Владислав Владимирович
... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Universitetsky 13, Moscow 119899, Russia, shev@sai.msu.ru . ... 1.Sternberg State Astronomical Institute, 119899, Moscow, Russia. shev@sai.msu.ru . ... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Moscow 119992, Russia, shev@sai.msu.ru . ... 119992 Moscow, Russia; . ... 2Sternberg Astronomical Institute, Moscow University, Moscow, 119992, Russia, . ... Moscow, 119992, Russia shev@sai.msu.ru . ...
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Ссылки http://selena.sai.msu.ru/Shev/Shev.htm -- 13.7 Кб -- 20.04.2015
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7. astro-ph authors/title/abstract search for 'galaxy merging' all years
... 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 ...
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Ссылки http://sed.sao.ru/lit/gal_merg.html -- 19.7 Кб -- 15.07.2001
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8. http://lnfm1.sai.msu.ru/SETI/koi/articles/abstr1.html
... Unlike the previous digital-only Messages, Arecibo-1974 and Evpatoria-1999, the TAM has complex, three-section structure with different forms of information. Section 1 represents coherent sounding radio signal with slow Doppler wavelength tuning to imitate transmission from Sun's center. ... Section 2 is an analog information and represents musical melodies, performed on the Theremin. ... There were seven musical compositions in the 1st Theremin Concert for Aliens. ...
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Ссылки http://lnfm1.sai.msu.ru/SETI/koi/articles/abstr1.html -- 3.2 Кб -- 16.10.2002
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9. Heliophysics, Internal structure and seismology
This home page belongs to small group of scientists working at . Sternberg Astronomical Institute which is a part of Moscow State University . ... Электронная библиотека научно-технической и художественной литературы (доступна только из ГАИШ) . ... Local staff . Dr. Edward Kononovich (konon -at- sai.msu.ru), Associate Professor . ... Dr. Sergey Ayukov (asv -at- sai.msu.ru), Research Fellow, Webmaster of the group . ... Joint seminar of Solar Studies Structure Group and Solar Photometry Group . ...
10. 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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11. PhD Thesis abstract
We investigate models for main-sequence and horizontal-branch (HB) stars constructed using the Carson opacities and make comparisons with models based on the Cox-Stewart opacities. ... The drop in the hydrogen-shell luminosity due to the helium-core expansion during HB evolution is greater than that obtained with the Cox-Stewart opacities. ... Studies of main-sequence (MS) stars lead to agreement with Stothers' (1974a,b, 1976) results for homogeneous models constructed with Carson opacities. ...
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Ссылки http://star.arm.ac.uk/~csj/phd.html -- 4.4 Кб -- 11.02.1997
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12. Vladimir Marsakov Abstracts
... 1) The MS lower envelopes for groups of stars with different metallicities turn out to be coincident. ... 4) The conformation of the kinematics of stars within narrow ranges ob b-y with the ages derived from isohrones reveals that, at Z < Z , the isohrone ages seem to be increasingly overestimated with growing b-y . ... At a given metallicity, they have a much narrower MS and the locus of their MS lower envelope seems to be brighter for the metal-rich group of stars. ...
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Ссылки http://ip.rsu.ru/~marsakov/abs/abst20.htm -- 4.8 Кб -- 02.02.2007
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13. Origin of the internal structures in HL Tauri jet (HH 151)
... The HH flow associated with young stellar object HL Tau has an exciting history and even until now the origin of some its features is not clear yet. ... Knotty structures of Herbig-Haro jets are common phenomena and knowing the origin of such structures is essential for understanding the processes of jet formation. ... In the flow detected compact knots with high (-150 km/s) and bow shape structures in front of those, with low radial velocities (-50 km/s). ...
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Ссылки http://www.sao.ru/Doc-en/SciNews/2012/Movses/ -- 5.1 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2012/Movses/ -- 5.1 Кб -- 02.10.2012
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[ Сохраненная копия ] Ссылки http://mavr.sao.ru/Doc-en/SciNews/2012/Movses/ -- 5.1 Кб -- 02.10.2012
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14. VLBI observations of the quasar 3C380
... There are result from two global VLBI observations at 3.6 cm spaced about 2 years. ... The analysis of the apparent motion, indication of the jet flow trajectory and the other implications for the CSS quasars are discussed. ... The quasar 3C380 ( ; thus 1 arcsec corresponds to 4 kpc for , ) is one of the most powerful radio sources (its radio luminosity at 2.7 GHz is ) ( Wilkinson et al. ... 3C380 is a member of the class of Compact Steep Spectrum (CSS) sources. ...
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Ссылки http://www.mrao.cam.ac.uk/yerac/owsianik/owsianik.html -- 11.9 Кб -- 08.12.2003
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15. PLDS-3, Chernogolovka, Russia, 2001 - Program, abstracts and proceedings
PROGRAM, ABSTRACTS and . PROCEEDINGS . Program, abstract and proceedings . ... Abstract Preparation . ... Last updates, 24 Nov 2001: . ... The third International Conference on Physics of Low-Dimensional Structures (PLDS-3) will be held on October 15-20, 2001 in Chernogolovka, Institute of Solid State Physics Russian Academy of Sciences, Moscow District. ... The scientific program covers a wide range of issues in modern physics of low-dimensional systems including the following topics: . ...
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Ссылки http://www.issp.ac.ru/plds3/conf.html -- 11.9 Кб -- 24.11.2001
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16. Space Research Institute (IKI) Seminar
... Future seminars . P a s t seminars . Seminar council . Stability of cold fronts in clusters of galaxies " . E. Churazov (IKI, MPA) . ... One of the insteresting results of Chandra and XMM-Newton observatories is the discovery of sharp structures in the X-ray surface brightness of galaxy clusters. These structures (a.k.a. cold fronts) are likely associated with the contacted discontinuities formed when a hot gas flows over a colder gravitationally bound gas cloud. ...
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Ссылки http://www.iki.rssi.ru/galeev/abs_eng/e040311.htm -- 4.3 Кб -- 04.03.2004
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/galeev/abs_eng/e040311.htm -- 4.3 Кб -- 04.03.2004
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17. Spatial Structure of NGC 6822: An Example for Statistical Modeling of
... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/pasztorl2.html -- 11.0 Кб -- 03.11.2000
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18. Stellarium: BigStarCatalogExtension::ZoneArray Class Reference
Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... BigStarCatalogExtension . ... BigStarCatalogExtension::ZoneArray Class Reference abstract . ... ZoneArray (const QString & fname , QFile *file, int level , int mag_min , int mag_range , int mag_steps ) . ... const int BigStarCatalogExtension::ZoneArray::level . ... const int BigStarCatalogExtension::ZoneArray::mag_min . ... const int BigStarCatalogExtension::ZoneArray::mag_range . ... const int BigStarCatalogExtension::ZoneArray::mag_steps . ...
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Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classBigStarCatalogExtension_1_1ZoneArray.html -- 38.1 Кб -- 28.02.2014
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19. g962f (Abstract)
... 2) Physics Department, University of Puerto Rico at Rio Piedras, P.O. Box 23343, San Juan, Puerto Rico 00931 . ... We report the density structure of the ultracompact HII regions G35.20-1.74, G9.62+0.19-E, and G75.78+0.34-H2O. The density profiles are derived from radio continuum emission at wavelengths from 6 to 0.3cm. In the case of G35.20-1.74, a cometary UC HII region with a core and a tail, the spectrum of the core varies as Snu~nu^(0.6), implying that the density structure is ne~r^(-2). ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/grad_uchii/abstract.html -- 2.9 Кб -- 11.09.2007
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20. ESO - Thesis Topic: Properties of kinematically decoupled structures in
... Science . ... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Properties of kinematically decoupled structures in Early-Type Galaxies . ... Science Users Information . ... ESO-MIDAS . ... ESO Science Newsletter . ... The project consists in measuring the stellar kinematics, stellar populations, dynamics, and morphological properties of the kinematically decoupled structures observed in the inner regions of Early-Type Galaxies. ... Return to list of thesis topics...
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Ссылки http://www.eso.org/sci/activities/thesis-topics/abstr-coccato2.html -- 27.8 Кб -- 10.04.2016
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