... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Parkes | ... Future ATNF Operations (Version 1) was released on the web in February 2008. During March and early April 2008 we visited universities around Australia to discuss the future operations plans with the Australian user community. ... Web forum feedback on ATNF Future Operations (Version 1) . ... Future ATNF Operations: Overview . ...

... Feedback in the Magellanic Clouds . ... Missions . ... Monday, October 5-Wednesday, October 7, 2015 . The goal of this workshop is to bring together the communities studying feedback in the Magellanic Clouds on both stellar and galactic scales. As the nearest gas-rich dwarf galaxies, the Magellanic Clouds offer a superb opportunity for studying the radiative, chemical, and mechanical feedback from star formation at high spatial resolution. ... October 5, 2015: Workshop begins . ...

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... Observatory . ... Science . User Portal . ... Science Users Information > Science Publications > Science Announcements > User Support Department Feedback Campaign . ... Science Users Information . Observing Facilities . ... Observing with ESO Telescopes . ... Data Handling and Products . ... Science Data Products Forum . ... Science Archive Facility . ... The User Support Department (USD) invites principal investigators and their Phase 2 delegates to participate in a user feedback campaign. ...

Thursday, June 24th, 2010 . ... Tags: site feedback . ... О лаборатории . ... Наши публикации . Публикации до 2008 . ... Публикации за 2009 . Публикации за 2010 . Публикации за 2011 . Публикации за 2012 . ... Статьи, публикации / 24 . ... December 2012 . November 2012 . October 2012 . August 2012 . June 2012 . April 2012 . February 2012 . January 2012 . ... June 2011 . ... June 2010 . ... Лаборатория лазерной интерферометрии is proudly powered by WordPress . ...

Guided by your suggestions, we desire to improve the Arecibo Observatroy operations to . better serve the needs of our users. Please complete and submit this form following your . ... Your comments will be reviewed by a number of NAIC-AO scientists and support staff. ... Receiver(s) used: . ... adequate . ... excellent . ... Please enter brief comments on the following: . ... ADDITIONAL COMMENTS: . If you have questions or problems with this form please send an email to . ...

We are very interested to receive your opinion, proposals and criticism concerning services provided by WDC-B as well as the whole WDC System. ... E-mail address: . Select and mark a level of your knowledge of the WDC System and experience in usage its services: . I know nothing of WDC System and never used it . I know of WDC System but never used it . I know of WDC System and used it a few times . I use WDC System on regular basis . ...

... Help . Before you report a problem you should check if it has already been reported in the help desk's SAS archive . If you decide to report a problem, then you can do so via the Observation Report (OR) form. Shortly thereafter you will be contacted by the XMM-Newton help desk . ... In most cases you'll be asked to send the following information, so you may consider enclosing it right away in your report (not all items apply in all cases): . ... Information about the CCF in use . ...

... Ever wonder how solar-mass stars form?. ... In order for material to accrete onto a protostar it has to lose angular momentum. The angular momentum of a large natal cloud leads to the formation of a circumstellar disk and inner accretion disk as the cloud collapses. ... Winds generated in the inner disk or close to the stellar surface (we don't know which) expel material along the disk rotation axis. ... This provides the highest resolution observational data on nearby young stars. ...

... Natalya V. Raguzova and Sergei B. Popov . ... We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 160 sources and provides information on names and spectral types of optical components, distances, on spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. ... Be/X-Ray Binaries and candidates in the Galaxy . Galactic sources: comments to the Table 1 . ...

... ISC Kosmotras . Top Management Founder of ISC Kosmotras - Dr. Vladimir A. Andreev News . Comments, Opinions Publications Dnepr Program . Dnepr launch record 17 August 2011. Cluster Launch of Dnepr LV 22 August 2013 KOMPSAT-5 Launch 21 November 2013. Dnepr Cluster Mission 2013 19 June 2014. Dnepr Cluster Mission 2014 6 November 2014. ... Mission profile SHM configuration Reliability Dnepr LV Performance Launch Sites . ... ISCK documents ISCK Photo Gallery Contact information . ...

... Метки: Twitter . ... 101) Байки из Фидо (7) Литература (16) Листая страницы прошлого Выберите месяц Апрель 2016 (2) Март 2016 (4) Февраль 2016 (4) Январь 2016 (5) Декабрь 2015 (4) Ноябрь 2015 (3) Октябрь 2015 (5) Сентябрь 2015 (5) Август 2015 (5) Июль 2015 (5) Июнь 2015 (4) Май 2015 (8) Апрель 2015 (5) Март 2015 (4) Февраль 2015 (4) Январь 2015 (7) Декабрь 2014 (7) Ноябрь 2014 (4) Октябрь 2014 (5) Сентябрь 2014 (8) Август 2014 (8) Июль 2014 (6) Июнь 2014 (7) Май 2014 (11) Апрель 2014 ...

. Euro-Asian Astronomical Society (EAAS): . Contact address: eaas@sai.msu.ru . Cochairpersons of EAAS: . Dr.Obridko Vladimir N. , obridko@izmiran.troitsk.ru . Dr. Ryabov Michael I., astro@te.net.ua . Dr. Samus Nikolai N., samus@sai.msu.ru . Secretary: . Dr. Valentina M. Chepurova, chep@sai.msu.ru . Executive officer: . Dr. Safar A. Gasanov, gasnizh@sai.msu.ru . Secretary: . Mrs. Vera L. Staerman, boch@sai.msu.ru . WebMaster: . webmaster .

... Events . ... Contact Us . ... Astronomy Summer Programme . ... Summer Events at Blackrock Castle . Reminder of Dr Carolyn Porco's lecture tour in Ireland : . Carolyn's lectures were completely booked up in Dunsink and BCO and the feedback from her talk is fantastic! ... For tickets contact Neil . Tuesday, 7 July 2009 11:40 . International Year of Astronomy, Ireland National Node . ...

... 5 1/ 2 Closing the feedback lo op: 1st option · Feedback efficiency 2NepEep f = Lp 4 3 w1 R 3 E1 w2 c E2 ( Eep E1 if E1 E2) · Pair pro duction rate Nep = · Soft (synchrotron from secondary pairs ) photon field: Eep 2 eB E2 1/2 f w w b , w2 = Es = 4 Es 2 mec2 mec · Hard ( inverse Compton from primary pairs ) photon field: 2 2 wb 3 R w1 , E1 = 3 2Ts wb = 4 R T ct 0 0 mec2 wb is thermal background energy density ...

. Main . Turbina . Rs485 driver . Microcodes . Documentations . CVS . Feedback . ASM Kislovodsk . Victor Kornilov . Olga Voziakova . Nicolas Shatsky . Sergey Potanin . Boris Safonov . Matwey Kornilov . Igor Gorbunov . Dmitry Cheryasov . Copyright 2004-2012.

... Galaxies, AGN, Cosmology . ... Blowin' in the wind: both `negative' and `positive' feedback in an obscured high-z Quasar . ... However, finding observational evidence of the effect of such AGN negative and positive feedback is still one of the main challenges in extragalactic astronomy . ... The results of this work are presented in the article " Blowin' in the wind: both `negative' and `positive' feedback in an obscured high-z Quasar ", Astrophysical Journal (in press; arXiv:1411.4208 ) . ...

... Sunday , October 6, 2013 Standard quasar-like AGN Standard AGN have: · · · · · Luminous accretion disk (with X-ray corona) Bright line emission (ionised by disk) Dusty obscuring torus (emits in IR/sub-mm) Orientation-dependent observed properties Sometimes, extended radio jets Sunday , October 6, 2013 Another class of AGN Other AGN , exemplified by weak radio ... Sunday, October 6, 2013 Summary · · · · · · Not all AGN follow the "standard" accretion disk picture. ...

Structure Formation : Bright side of the Universe Anatoly Klypin New Mexico State University Also: Stefan Gottloeber (Astrophysikalisches Institut Potsdam) Gustavo Yepes (UAM, Madrid) Cosmological ... -body+hydro simulations Codes: SPH + TREE AMR + shock capturing hydro Physical processes: Compton cooling/heating on CMB Radiative gas cooling Star formation with simple approximations Metal enrichment Energy/momentum feedback from young stars and SN Galaxies too concentrated. ...

... This script also shows a simple but crude way of displaying more feedback while operating: it opens the DIS Expose window. ... As always, get permission to use DIS before commanding it. import TUI.TUIModel def init(sr): """Open the DIS Expose window so the user can see what's going on.""" tuiModel = TUI.TUIModel.getModel() tuiModel.tlSet.makeVisible("None.DIS Expose") def run(sr): """Sample script to take a series of DIS calibration images and demonstrate looping through data in Python. ...