Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Найдено документов: 431301 (180 сайтов) ---- Время поиска: 1.33сек.   

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | След.

Показаны документы, содержащие фрагменты текста из документа
http://www.mrao.cam.ac.uk/projects/surveys/snrs/snrs.G74.0-8.5.html.

1. G189.1+3.0
... Flux density at 1 GHz (/Jy): 160 . ... Radio: Limb-brightened to NE, with faint extension to the E. Optical: Brightest to the NE, with faint filaments outside the NE boundary. ... Fesen 1984, ApJ, 281, 658. ... ADS . ... 151 MHz observations (1'.2?3'.1) and Half-Mile Telescope at 1.4 GHz (2'.1?5'.4). ... Radio, IR, optical, UV and X-ray comparison, including VLA at 1.6 GHz (3".8?3".3 and 40''). ... 1988, ApJ, 335, 215. ... IR observations of shocked O 2 . ... Observations of shocked molecular...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs/snrs.G189.1+3.0.html -- 13.6 Кб -- 10.04.2016
Похожие документы
Еще в разделе: (Показать все результаты (>5184) - www.mrao.cam.ac.uk/ )

2. Radio survey for new compact HII regions
... 227Wink This paper containes an investigation of 91 sources which appear to be point sources when observed with the angular resolution of the 100-m telescope at 4.9 GHz, teta_a = 2.6', and which we expected to be HII regions. The basic search list was prepared from the 4.9 GHz survey of the galactic plane by Altenhoff et al. ... In the present paper we list 4.9 GHz flux densities only for sources for sources for which we present new observations. ... source structure indicated . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/HII_Wink.html -- 4.8 Кб -- 18.03.2015
Похожие документы

3. A Spitzer Space Telescope Far-Infrared Spectral Atlas of Compact Sources in the
We present far-infrared spectra, ЮЛ = 52-93 ЮМm, obtained with the Spitzer Space Telescope in the spectral energy distribution mode of its MIPS instrument, of a representative sample of the most luminous compact far-infrared sources in the Large Magellanic Cloud (LMC). ... First, we introduce a spectral classification scheme. ... The efficiency of photoelectric heating in the interfaces of ionized gas and molecular clouds is estimated at 0.1%-0.3%. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2010AJ....139...68V.html -- 6.0 Кб -- 21.01.2016
Похожие документы

4. casacore: images/Regions/WCLELMask.h Source File
... Classes . ... Regions . ... 00001 //# WCLELMask.h: Class to define a mask as a LEL expression 00002 //# Copyright (C) 2000,2003 00003 //# Associated Universities, Inc. ... /# National Radio Astronomy Observatory 00023 //# 520 Edgemont Road 00024 //# Charlottesville, VA 22903-2475 USA 00025 //# $Id: WCLELMask.h 20615 2009-06-09 02:16:01Z Malte.Marquarding $ 00026 00027 00028 00029 #ifndef IMAGES _ WCLELMASK _H 00030 #define IMAGES _ WCLELMASK _H 00031 00032 //# Includes 00033 #include images /...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/WCLELMask_8h_source.html -- 29.3 Кб -- 14.02.2011
Похожие документы

5. Source non-overlap algorithm
... region (region-7.9.3) [xmmsas_20080701_1801-8.0.0] . ... Sources which lie close to each other may generate event-extraction regions which overlap. ... If the user selects shrinkconfused =`yes', and provided that the source region shape is circular not elliptical (true if radiusstyle is not equal to `contour', or if radiusstyle =`contour' but nosrcellipse =`yes'), the task will reduce the radii of pairs of overlapping source regions until they no longer overlap. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/region/node9.html -- 5.2 Кб -- 02.07.2008
Похожие документы
Еще в разделе: (Показать все результаты (>11295) - xmm.vilspa.esa.es/ )

6. Select a circle around the central point source
Next: A box, to include Up: To produce a region Previous: To produce a region . select cursor and circle . When in the image window, the mouse now has a box shape with an arrow at the upper left corner. The mouse buttons act as follows: . LEFT - to move the center of the circle at the position of the arrow point. ... RIGHT - idle. center the circle at the point source by positioning the arrow point and clicking on the LEFT mouse button. A circle will appear at the arrow position. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node62.html -- 5.9 Кб -- 01.10.2012
Похожие документы

7. VLBApls source sample
... The VSOP Survey Continuum Source List . The radio sample for the VSOP continuum survey was defined to include all extragalactic radio sources with: . a total flux density at 5 GHz, S>=1.0 Jy . ... The sample also included all sources in the sky with a 5 GHz flux density S>5 Jy, regardless of spectral index and galactic latitude. ... The source would then be included in the VSOP sample (three of the sources were found with a flux density above 1 Jy and added to the sample). ...
[ Сохраненная копия ]  Ссылки http://www.vsop.isas.ac.jp/VLBApls/sample.htm -- 4.1 Кб -- 17.10.2000
Похожие документы
Еще в разделе: (Показать все результаты (>470) - www.vsop.isas.ac.jp/ )

8. The Cross-correlations
... The actual cross-correlations were done as follows: north of WGACAT was correlated with the GB6 catalog with a correlation radius of one arc minute. ... We therefore cross-correlated WGACAT with the GB6 and PMN radio catalogs with a 1.5 arcmin radius. ... As a result of this experiment, we then added to the WGACAT/PMN candidate list the 29 unclassified sources obtained from the 1.5 arcmin correlation and having PSPC offsets arcmin, ratio between X-ray/radio offset and positional error , and . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~ppadovan/survey/dxrbs_paper/node5.html -- 11.3 Кб -- 03.12.2003
Похожие документы

9. The BD+40 region (Abstract)
... Near-IR broad-band imaging of V1318 Cygni reveals the presence of two distinct stellar components oriented north-south, a result recently reported by Aspin et al. ... The distribution of the high density molecular gas traced by the CS J emission is highly concentrated around V1318 and V1686 Cygni, while the total column density of gas traced by the J shows a ridge morphology centered on these sources. ... A molecular outflow has been detected in CO J . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/bd40_fig_aa/abstract.html -- 4.1 Кб -- 11.09.2007
Похожие документы

10. A New PROS Task for Calculating HRI Source Intensities or Upper Limits
... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/chenj.html -- 11.4 Кб -- 03.11.2000
Похожие документы

11. Grav_lens
Porcas (MPIfR, Germany), Garrett (JIVE, Netherlands), Patnaik (Canada) & Nair (RRI, India) have attempted to make a ``definitive'' high-resolution study of the gravitational lens system, 2016+112, using an 18-station Global VLBI Array run at 5 GHz, including the Arecibo 305-m telescope. ... There are 3 image ``regions'' (A, B & C) spread over an area of 4 arcsec. Previous VLBI observations (e.g., Garrett et al., ... Arecibo-VLBA_Saint Croix baseline. The bandwidth is 16 MHz, the . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/aovlbi/Gravitational_lens/Grav_lens.html -- 5.2 Кб -- 16.03.2004
Похожие документы

12. Radio sources identfification
... LABORATORY OF RADIO ASTRONOMICAL OBSERVATIONS . Radio sources identification is one of the most important tasks of the current radio astrophysics. ... Optical idetification. ... Optical identifications of subsample of steep spectra radio sources from RC catalog using 6m SAO telescope of SAO RAS: optical observations. ... Astronomy Reports. ... Identification of radio sources with data of various radio catalogs allows one to construct continual spectrum of the object and its radio structure. ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/lran/vo/rs_idE.html -- 8.9 Кб -- 01.10.2012
Похожие документы

13. lsst.coordConv: include/coordConv/coordConv.h Source File
lsst.coordConv љ unknown . ... Classes . Files . FileљList . All љ Classes љ Namespaces љ Files љ Functions љ Variables љ Typedefs љ Enumerations љ Enumerator љ Pages . include . ... 3 љ #include " coordConv/physConst.h " . 4 љ #include " coordConv/mathUtils.h " . 5 љ #include " coordConv/time.h " . 6 љ #include " coordConv/angSideAng.h " . 7 љ #include " coordConv/rotEqPol.h " . ... 10 љ #include " coordConv/coord.h " . ... 13 љ #include " coordConv/coordSys.h " . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/coordConv/html/coord_conv_8h_source.html -- 10.1 Кб -- 07.05.2015
Похожие документы

14. astro-ph
... astro-ph . ... Statistical Characterization of the Chandra Source Catalog . ... The first release of the Chandra Source Catalog (CSC) contains ~95,000 X-ray sources in a total area of ~0.75% of the entire sky, using data from ~3,900 separate ACIS observations of a multitude of different types of X-ray sources. ... In addition to these traditional catalog elements, for each X-ray source the CSC includes an extensive set of file-based data products that can be manipulated interactively. ...
[ Сохраненная копия ]  Ссылки http://vo.astronet.ru/arxiv/?get_articles=1&author=He -- 15.7 Кб -- 13.04.2016
Похожие документы
Еще в разделе: (Показать все результаты (>40102) - vo.astronet.ru/ )

15. Lecture XVIII.
Overall 2 % of the total available thermal energy in this region heats water for steam . How many years can this source provide power for electricity generation at the rate of 2000 MW per year? Total Capacity required is 2000 Mw per year/0.02 = 100,000 MW per year . Since 1 Joule = 1 Watt per second then 100,000 MW per year is equivalent to 3.15 x 10^18 Joules per year (there are 3.15x10^7 seconds in a year) . ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/ph162/l18.html -- 6.1 Кб -- 23.02.1995
Похожие документы

16. Martian mini station (MMS)
... Meteorological, seismic and electromagnetic observations on the surface of the Mars with the network of MMSs. ... The MMS equipment includes all devices needed for autonomous MMS operation and ensures operability in the whole temperature range during the Martian year in different regions of the Martian surface. ... The radio system (transmitter, receiver and antenna) is capable to transmit information to the Martian orbiter with 128 kbit/s and receive control commands. ... 3-axial accelerometer; . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/innov/eng/mms7.htm -- 3.3 Кб -- 02.10.2006
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/innov/eng/mms7.htm -- 3.3 Кб -- 02.10.2006
Похожие документы

17. Stellarium: core/StelSphericalIndexMultiRes.hpp Source File
... 40 љ template < class FuncObject> void processIntersectingRegions ( const SphericalRegionP & region, FuncObject& func) const . ... 44 љ const RootNode* node = treeForRadius[i-1]; . ... 87 љ const Vec3d & c0 = triangle.getConvexContour().at(0); . ... 195 љ template < class FuncObject> void processIntersectingRegions ( const Node& node, const SphericalRegionP & region, FuncObject& func) const . ... 212 љ template < class FuncObject> void processAll ( const Node& node, FuncObject& func) const . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/StelSphericalIndexMultiRes_8hpp_source.html -- 38.5 Кб -- 28.02.2014
Похожие документы

18. Detection of polarized radiation sources with unusual spectral characteristics
... Solar flare activity is produced by the processes of accumulation and release of energy in an active region. ... In the framework of study of solar active regions, producing powerful flares the researchers from the RATAN-600 radio telescope have detected sources with features in the form of a sharp drop in the intensity of polarized radiation in various parts of the recorded frequency range (2-16GHz), sometimes changing the sign of polarization. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2011/Bogod/ -- 4.0 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2011/Bogod/ -- 4.0 Кб -- 02.10.2012
Похожие документы

19. Atomic data for Stellar Atmospheres: lte_lines
For calculating model spectra of early-type helium stars in LTE, we maintain a database of atomic data for, mostly, blue-visual absorption lines of light elements. The data is sorted with one file for each ion. ... III = ++ . ... It will work on both complete linelists (including the atomic data at the start and references at the end) or raw ion files (such as Ni2.d). ... A Fortran utility to convert linelists downloaded from the Vienna Atomic Line Database into the new QUB format. synspec_qub . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/lines/lte/html/lines.lte.html -- 10.4 Кб -- 15.11.2001
Похожие документы

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | След.


Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам

Комментарии, вопросы? Пишите: info@astronet.ru или сюда

Rambler's Top100 RFBR Яндекс цитирования