Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Найдено документов: 270423 (166 сайтов) ---- Время поиска: 0.46сек.   

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

Показаны документы, содержащие фрагменты текста из документа
http://www.arcetri.astro.it/irlab/luna/firpo/firpo_publ.html.

1. FIRPO Publications
... Last modified on August 19, 1996 by A. Richichi . ... Hamilton, D.P., Herbst, T.M., Richichi, A., B?hnhardt, H., Ortiz, J.L. 1995, '' Calar Alto observations of Shoemaker-Levy 9: characteristics of the H and L impacts '', Geophysical Research Letters, 22 , 2417. ... Hamilton, D. P., Herbst, T. M., B?hnhardt, H., Ortiz-Moreno, J. L., Richichi, A., Calamai, G. 1995, `` Calar Alto Observations of the A, H, L, Q1 and Q2 Impacts '', Proceedings of the XXIInd General Assembly of the IAU, den Haag 15-27...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/luna/firpo/firpo_publ.php -- 11.1 Кб -- 04.02.2013
Похожие документы

2. Supernova 2009js in NGC 918
Supernova 2009js in NGC 918 . This page is devoted to information on Supernova 2009js in NGC 918 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. Discovered independently by Lick Observatory Supernova Search (USA) and Koichi Itagaki (Japan). ... 2009/10/11.44 . 17.2 . ... Joseph Brimacombe . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/sn2009/sn2009js.html -- 8.2 Кб -- 13.02.2011
[ Сохраненная копия ]  Ссылки http://www.rochesterastronomy.org/sn2009/sn2009js.html -- 8.4 Кб -- 19.04.2014
Похожие документы
Еще в разделе: (Показать все результаты (>860) - www.rochesterastronomy.org/ )

3. ESO - 8th VLTI Summer School: High angular resolution in astrophysics: optical
... Science Publications > Science Announcements > 8th VLTI Summer School: High angular resolution in astrophysics: optical interferometry from theory to observations . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... ESO Data . ... ESO HST Image Galleries . ... ESO Data Access Policy . ... ESO Science Newsletter . ... Optical/infrared long-baseline interferometry has reached a new stage with the advent of multi-telescope arrays accessible to a broad community of astronomers, most notably VLTI . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/publications/announcements/sciann15050.html -- 23.9 Кб -- 10.04.2016
Похожие документы
Еще в разделе: (Показать все результаты (>27776) - www.eso.org/ )

4. Arecibo Radar Discovers Triple Near-Earth Asteroid
Image credit: Michael Nolan, Arecibo Observatory. These radar images of near-Earth asteroid 2001 SN263 were obtained on 2008 Feb 12 and 13. ... Image from Feb 12 . ... First near-Earth triple asteroid discovered by Arecibo Observatory . ... was discovered this week by astronomers at the sensitive radar telescope at Cornell University?s Arecibo Observatory in Puerto Rico. ... For example, Arecibo has discovered more than half of the near-Earth binary asteroid systems discovered since 1999. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~pradar/asteroids/2001SN263/ -- 7.7 Кб -- 23.02.2008
Похожие документы

5. First X-Rays From a Comet Discovered
A team of U.S. and German astrophysicists have made the first ever detection of X-rays coming from a comet. ... Following the initial detection, the team reported repeated X-ray emissions from the comet over the next 24 hours. ... One preliminary theory is that X-ray emission from the Sun was absorbed by a cloud of gaseous water molecules surrounding the nucleus of the comet, and then were re-emitted by the molecules in a process physicists call "fluorescence." ... Comets . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/solar/eng/hyakutak.htm -- 5.3 Кб -- 15.10.1997
Похожие документы

6. Departement of Quantum Astrophysics
. Departement of Quantum Astrophysics . Head: Kurt V.G. , Prof. ultraviolet spectroscopy of planetary upper atmospheres and interplanetary/interstellar medium; . observations of gamma-bursts and optical identification of their sources; . long-base optical interferometry. Staff: .
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/mdiv/qad/qad.htm -- 1.9 Кб -- 04.12.1997
Похожие документы
Еще в разделе: (Показать все результаты (>190) - www.asc.rssi.ru/ )

7. The Optical Counterparts to Galaxies in the Cen A Group Discovered by HIPASS
... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... The Optical Counterparts to Galaxies in the Cen A Group Discovered by HIPASS . ... This group of galaxies was recently the subject of a separate and thorough optical survey (CУДtУ? et al. 1997), and thus presented an ideal comparison for us to test the survey performance. ... Six of the new members are previously uncatalogued galaxies, while four were catalogued but assumed not to be group members. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/16_1/knezek/paper/index.html -- 52.9 Кб -- 08.04.2016
Похожие документы

8. Journal "Peremennye Zvezdy"
Peremennye Zvezdy", . ... Find.Chart . ... GSC 04516-02121 . ... The new variable star 2MASS J00511854+5022580 (indicated as V in the finding chart) is inside the field of view of the known variable star V364 Cas. ... The new variable star GSC 04516-02121 (indicated as V in the finding chart) is inside the field of view of the known variable star V405 Cep. ... The variable star 2MASS GSC 00770-00523 (indicated as V2 in the finding chart) is inside the field of view of the known variable star AV CMi. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1238571 -- 14.9 Кб -- 27.02.2010
Похожие документы

9. APOD: 2005 December 5 - Ice Fountains Discovered on Saturns Enceladus
Discover the cosmos! ... 2005 December 5 . Fountains Discovered on Saturn's Enceladus . Credit: Cassini Imaging Team , SSI , JPL , ESA , NASA . Explanation: Fountains of ice shoot out from Saturn's moon Enceladus. Clear discovery images of the fountains were made using observations from the robot Cassini spacecraft currently orbiting Saturn . During a recent pass, Cassini was programmed to look back toward the Sun where Enceladus would appear as a thin crescent . ... About APOD | ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap051205.html -- 5.2 Кб -- 02.10.2012
Похожие документы

10. Astrophysics Group VSA
... Astrophysics Group . ... VSA . ... CAT . ... The Very Small Array is a custom-built radio telescope (operating between 26-36 GHz), designed expressly to make high resolution observations of the cosmic microwave background (CMB) radiation on angular scales around and below one degree. ... The VSA has been operated in ?compact array? and ?extended array? configurations (see the technical description below) and data collected to achieve high sensitivity in both regimes have been analysed. ... 1.75 GHz)...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/outreach/radio-telescopes/vsa/ -- 20.2 Кб -- 10.04.2016
Похожие документы

11. http://www.stsci.edu/ftp/instrument_news/GHRS/Ghrs_handbook/v4.1/doppler_advisory_text.ps
GHRS Instrument Handbook 4.1 103 Addendum 1 Advisory : Potential Data Corruption A1.1 The Problem : Incorrect Doppler Compensation 104 A1.2 How to Tell if Data Are Affected 105 A1.3 Fixing the Problem 105 Advisory : Potential Data Corruption Advisory : Potential Data Corruption Advisory : Potential Data Corruption GHRS Instrument This discussion pertains not just Cycle 4 but to current observations and all previously obtained GHRS data. ...
[ Текст ]  Ссылки http://www.stsci.edu/ftp/instrument_news/GHRS/Ghrs_handbook/v4.1/doppler_advisory_text.ps -- 69.8 Кб -- 26.09.1997
Похожие документы

12. On the problem of high spectral resolution observations of faint objects
... December 21, 1997 . ... Advantages are briefly discussed of gaining in spectral resolution, which is accompanied by losses in signal level, as compared with the attempts to improve the accuracy of measurement of line parameters by means of rising the S/N ratio alone with increasing the exposure time. To partially solve the problem of observations of faint objects at the BTA a new design echelle spectrometer is propos