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181. AAL Homepage
... The spectrum of the brightest star, our Sun, shows several dark gaps perpendicular to the flow of it’s colours (figure 1). These so called spectral absorption lines where discovered in 1802 by the English scientist William Wollaston. ... Some stars as Pollux show a spectrum similar to that of our sun with strong Ca II and Fe II lines, others as Sirius or Vega show strong absorption lines of hydrogen, others, as Mira show very complicated spectra due to molecular absorption lines (see figure 5). ...
[ Сохраненная копия ]  Ссылки http://www.aal.lu/SPECIAL_TOPIC/6/ -- 44.4 Кб -- 09.04.2016
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182. http://www.jsc.nasa.gov/history/oral_histories/CarruthersGR/GRC_BIO.pdf
NAME: Dr. George R. Carruthers MARITAL S TATUS : Unknown RESIDENCE: Washington, DC E DUCATIONAL BACKGROUND: BS in Aeronautical Engineering , University of Illinois , 1961 MS in Nuclear Engineering , University of Illinois , 1962 Ph.D. in Aeronautical Astronautical Engineering (Minor in Physics and Astronomy ), University of Illinois , 1964 PRE- ...
[ Текст ]  Ссылки http://www.jsc.nasa.gov/history/oral_histories/CarruthersGR/GRC_BIO.pdf -- 15.5 Кб -- 13.10.2006
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183. http://site2010.sai.msu.ru/static/doc/FKerber_site2010.pdf
... European Southern Observatory at Site 2010 Kislovodsk Collaboration University of Lethbridge, Canada ­ R. Querel, D. Naylor, G. Tompkins U. Valparaiso ­ A. ChacСn, O. Cuevas, M. Cure, L. Cortes, M. Caneo, L. Illanes ­ J. ThomasOsip, G. Prieto ­ A. OtАrola, M. SchЖck, T. Travouillon ­ R. Hanuschik, M. Sarazin, C. Guirao, G. Avila, G. Lo Curto, I. Saviane, A. Pizarro, G. Ihle, J. Navarette, A. Smette, D. Rabanus Site 2010 Kislovodsk, Oct 5th, 2010 2 GMT, Las Campanas TMT ESO F. Kerber et al. ...
[ Текст ]  Ссылки http://site2010.sai.msu.ru/static/doc/FKerber_site2010.pdf -- 2041.8 Кб -- 18.10.2010
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184. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0098-1-1.pdf
... 6 Table 5: Fit of shifts of individual lines with Solar Angle a -0.7±0.7 .. ... Table 8: Line shifts : RGS2 Order 1 Obsid 121920 123720 126130 123940 123940 123940 123720 133120 133120 134520 134540 134540 134720 134520 134540 134540 134521 134521 134521 134521 134540 134720 134521 134521 134522 134522 134522 134522 134522 Target Capella AB Dor AB Dor Procyon Procyon Procyon AB Dor AB Dor AB Dor AB Dor HR 1099 HR 1099 Capella AB Dor HR 1099 HR 1099 AB Dor AB Dor AB ...
[ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0098-1-1.pdf -- 425.8 Кб -- 25.02.2015
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185. http://sn.sai.msu.ru/~sil/preprints/iau245sil.pdf
... Panoramic spectroscopy of the sample of 80 nearby lenticular galaxies is presented. ... By comparing the subsample of the S0s with the chemically distinct nuclei to the total sample of nearby S0s (Fig. 1), we have assured that the chemically distinct nuclei are always younger than the surrounding bulges: the mean age difference between the chemically distinct nuclei and their surrounding bulges is 2.8 Gyr while the age difference between the nuclei and the bulges for the whole sample is only 1 Gyr. ...
[ Текст ]  Ссылки http://sn.sai.msu.ru/~sil/preprints/iau245sil.pdf -- 195.3 Кб -- 23.01.2010
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186. http://www.2dfquasar.org/Papers/2001MNRAS.322L..29C.pdf
... 322, L29 ± L36 (2001) The 2dF QSO Redshift Survey ± V. The 10k catalogue S. M. Croom,1w R. J. Smith,2 B. J. Boyle,1 T. Shanks,3 N. S. Loaring,4 L. Miller4 and I. J. Lewis1 1 2 3 4 Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD Department of Physics, University of Durham, South Road, Durham DH1 3LE Department of Physics, Oxford University, 1 Keble Road, Oxford OX1 3RH Accepted 2001 March 7....
[ Текст ]  Ссылки http://www.2dfquasar.org/Papers/2001MNRAS.322L..29C.pdf -- 372.0 Кб -- 04.03.2004
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187. Near Earth Asteroid Rendezvous (NEAR)
... Р?С?С?С?Р?Р?Р?Р?РеС?Р?С?Р?РеР? ... Launched on February 17, 1996, the Near Earth Asteroid Rendezvous (NEAR) mission is to be the first of NASA's Discovery missions, a series of small-scale spacecraft designed to proceed from development to flight in under three years for a cost of less than $150 million. ... The ultimate goal of the mission is to rendezvous with and achieve orbit around the near Earth asteroid 433 Eros in February, 1999, and study the asteroid for approximately one year. ...
[ Сохраненная копия ]  Ссылки http://astro-all.narod.ru/asteroids/near.htm -- 15.3 Кб -- 09.04.2016
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188. Народ.Ру: Высокое спектральное разрешение, 200000>R>20000
Высокое спектральное разрешение, 200000>R>20000 . HIRES - эшелле спектрограф 10м телескопа Keck . HRS - оптоволоконный эшелле спектрограф 9м телескопа HET . ... CELESTIA - оптоволоконный эшелле спектрограф 9м телескопа SALT . PEPSI - оптоволоконный эшелле спектрограф-поляриметр 2х8.4м телескопа LBT . ... HROS - оптоволоконный эшелле спектрограф 8.1м телескопа Gemini S . ... UCLES и UHRF - эшелле спектрографы высокого и сверхвысокого разрешения 3.5м телескопа ААТ . ...
[ Сохраненная копия ]  Ссылки http://astrospectra.narod.ru/R20links.html -- 22.2 Кб -- 09.04.2016
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189. http://www.aaa.org/EyepieceFiles/aaa/2012_02_February_Eyepiece.pdf
... This accuracy allows HARPS to detect planets with masses slightly greater than the Earth. Among the 50 new HARPS planet discoveries announced in September, the one that garnered the most attention orbits the star HD 85512 (aka Gliese 370), 36 light-years awa y in the southern constellation Vela. The planet, given the prosaic designation HD 85512 b, has a mass of about 3.6 times that of Earth and orbits its star, an orange K-type dwarf, in 59 days. ... Happy People Dancing on Planet Earth." ...
[ Текст ]  Ссылки http://www.aaa.org/EyepieceFiles/aaa/2012_02_February_Eyepiece.pdf -- 2482.5 Кб -- 14.10.2015
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190. http://www.princetonastronomy.org/newsletters/12_2004sidereal.pdf
... A Splendid Visit to the Star Hill Inn, New Mexico In November I was fortunate to visit, with my wife Carol, one of the southwest's premier astronomy retreats, the Star Hill Inn north of Las Vegas, NM. ... I spent four nights observing under transparent skies which, when cloud free (one of four nights was pristine while the other three were clear about half the night), revealed magnitude 6.5 stars and, for example, M33 as a naked eye object! ... These efforts should not go unnoticed by AAAP members. ...
[ Текст ]  Ссылки http://www.princetonastronomy.org/newsletters/12_2004sidereal.pdf -- 2181.1 Кб -- 09.12.2004
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191. http://www.vista.ac.uk/Files/docs/PublicSurveys-ESO-Messenger-no127_Arnaboldi.pdf
Telescopes and Instrumentation ESO Public Sur veys with the VST and VISTA The ESO Sur vey team: Magda A rnaboldi, Mark J. Neeser, L aura C. Parker, Piero Rosati, Marco Lombardi, JЖrg P. Dietrich, Wolfgang Hummel A n e w c h a p te r f o r E u r o p e a n a s t r o n o m y w i l l s o o n b e g i n w i t h d e d i c a t e d s u r ve y telescopes in the optical and near-infrar e d . ... This sur vey will also be complemented with near-infrared data from the VHS VISTA sur vey. ...
[ Текст ]  Ссылки http://www.vista.ac.uk/Files/docs/PublicSurveys-ESO-Messenger-no127_Arnaboldi.pdf -- 1405.9 Кб -- 14.06.2012
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