... 1 Time (UT) 11:50 X-ray BP behaviour Magnetic fragment behaviour A small bipolar region locates at northwest of a positive dominant region. Both positive and negative fragments move toward each other in the bipolar region. ... A few strong negative fragments from southeast move toward the dominant positive fragments. Both polarities in the bipolar region become less and weaker. ... The negative fragments in the bipolar region become very weak and have a certain distance from the positive one. ...

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• http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/121107/121107_07.pdf
• http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/130109/130109_02.pdf
• http://star.arm.ac.uk/highlights/2012/603/bp_mag/VisualAnalysis/121107/121107_05.pdf

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

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Тема : Хвостатые гостьи V (информация для наблюдения комет) .. Показать сообщение отдельно . ... Хвостатые гостьи .. ... после того, как ISON приплыл мимо нас, земля находится на орбитальной траектории, которая пройдет через след частицы кометы (тот, который ISON оставил позади, когда это приближалось к солнцу и это случайно встретит или вокруг 12 января - 15, 2014 . ... лучшее время наблюдения 22:00 LDT (Northern hemisphere 45њ North) .. - радиант расположен вблизи Al'dzhabkhakh (30-Eta Leonis, ? ...

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. Please standby and you will be automatically connected to the new location of the unframed Supernova page. Or, click on the link above. If you have questions or problems, please email me at David Bishop dbishop@vhdl.org . Last modified: Mon Aug 27 12:40:15 EDT 2001

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• Supernova 2000B in NGC 2320
• Supernova 2011iy in NGC 4984
• Supernova 2009I in NGC 1080

Next: Current Challenges Up: Scientific Results from Deconvolved Previous: HST Science: Structure . ... The presence of strong central concentrations in the starlight of galaxies is important in understanding their dynamics, and in searching for the massive compact objects thought to exist in (at least) active galactic nuclei. ... The core of the Andromeda galaxy, M31, has also been suspected to harbor a massive central object from ground-based spectroscopic data (Dressler , 1988, Kormendy 1988). ...

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• Absorption line spectra of the UV bright z=2.4 QSO HE 1122-1649
• Surface Brightness Profiles
• WFPC2 Instrument Handbook Update

... 27.07.2011 . ... Comet Garradd was discovered two years ago by Gordon Garradd in Australia , and is currently visible through a small telescope at visual magnitude nine. Officially designated C/2009 P1 (Garradd), the comet will likely continue to brighten, with recent projections placing it at peak magnitude six or seven in February 2012, just below naked eye visibility. ... July 2011 . ... 2011 2012 . ... Publications with keywords: comet - Solar System . ... Comet Lovejoy over The Great Wall . ...

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• Journal "Peremennye Zvezdy"
• Another Nearby Supernova in the Whirlpool Galaxy
• Unusual Bright Soil on Mars

Race to the Planets Family Event Sample Agendas Family ASTRO Leader Kits and Guides are designed to contain enough materials and activities for two full family events. ... What's Next: As families leave, make sure they know about the date and time for your second Race to the Planets session and that you'll want to know how they did playing the "Surfing the Solar System" game. ... If there are any planets visible in the night sky, a nice follow up to this family event is a planet observing session. ...

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• ASP: Eclipse Watching: Making a Solar Filter
• ASP: Family ASTRO: Take-Home Activities(Games and Kits for Families and...
• ASP: Focus on Education: The Key to Success in Astronomy

Check out the new images (Jan 18-25) and (Jan 26-Feb 05) of the comet by Rob McNaught. ... Every few years a comet becomes bright enough to be easily seen with the naked eye but only every decade or so are these comparable with comets like Halley. ... Before Jan 13, the comet is not visible in the Australian sky after sunset. ... SOHO images . ... On Jan 12 at approximately 09:00 UT (8pm NSW time), comet C/2006 P1 McNaught appears at the 11 o'clock position in the images. ... STEREO images . ...

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• The High-Z SN Search Description
• Siding Spring Survey
• Sky Brightness

... The storm began quite unexpectedly. The strongest geomagnetic storm for the last seven months began on Earth almost precisely at the same time as the solar eclipse reached its maximal stage, the culmination of which occurred at GMT 02:35 (06:35 Moscow time). ... Oscillations of such amplitude in the magnetic field have not been observed since October, 11th of last year, which is more than seven months ago. ... We can only add that the magnetic storm lasted approximately 9 hours. ...

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• The CORONAS-PHOTON has registered the formation of the Sun's southern belt of
• Project's diary
• Solar activity hits a new low

To continue a command onto another line enter a ' \\ ' (backspace) character and then press <Return> . You can then continue entering the command. For example: rcp ubik:/home/roger/recipe.ps .; Return> lpr -Pps3 #6m recipe.ps . This copies the file recipe.ps from the home directory of the user roger on the remote host ubik to the users current directory. ... If you are using the Bourne, BASH or Korn shell a > character appears as a prompt at the start of the second command line. ...

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Hubble Observations Shed New Light on Jupiter Collision . Was it a comet or an asteroid? ... Their initial findings, combined with results from other space-borne and ground-based telescopes, shed new light on Jupiter's atmospheric winds, its immense magnetic field, the mysterious dark debris from the impacts, and the composition of the doomed comet itself. ... Hubble's ultraviolet observations show the motion of very fine impact debris particles now suspended high in Jupiter's atmosphere. ...

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• Educator's Guide to Moon Phases
• Arcetri Solar Physics Group: Solar Activity
• Educator's Guide to The Inverse Square Law

... 2006 April 6 . Unusual Bright Soil on Mars . Credit: Mars Exploration Rover Mission , Cornell , JPL , NASA . Explanation: What is this bright soil on Mars? Several times while rolling across Mars, the treads of the robotic rover Spirit have serendipitously uncovered unusually bright soil. ... The physics and chemistry instruments on Spirit have determined the soil, shown above , contains a high content of salts including iron-bearing sulfates . ... About APOD | ...

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• APOD: 2011 June 5 - Another Nearby Supernova in the Whirlpool Galaxy
• APOD: 2002 March 7 - Comet Ikeya-Zhang Brightens
• APOD: 2015 September 16 - Bright Spots Resolved in Occator Crater on Ceres

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 . ...

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• Uranus' Moon Umbriel
• The Acceleration of the Aurora
• Ion Rockets

... The Galactic low-mass X-ray binary GS 2023+338 was discovered during the burst on May 22, 1989 with the Japanise satellite Ginga (aka Galaxy). The flux reached 17 crabs (this unit of flux measurement is an bright X-ray source, Crab Nebula) at 10-35 keV. ... No other radio telescope worldwide carried out multi-frequency measurements. ... Upon 14 days the radio flux fell below the detection level at the RATAN-600 in relation to the decrease of the X-ray flux. ...

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• Galaxy sector, archive 2014
• New LBV Stars in the Andromeda Galaxy

... 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. ...

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Next: Sky models Up: Reductions --- at Previous: Robust fits and . ... Sky values may have already been subtracted (e.g., in CCD measurements or other data marked as RAWMAG instead of SIGNAL.) DARK CURRENT: Dark current is usually a strong function of detector temperature. If you have regulated the detector temperature, then only a weak time dependence might be expected --- perhaps only a small difference from one night to the next, or a weak linear drift during each night. ...

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• HyperLEDA documentation: HyperLEDA: catalogue of agnclass (a109)
• Image quality-contrast
• Nonlinearity

... Orbits in Space . ... The ion rocket is another means of providing thrust, more gradually but also more efficiently than a conventional rocket. ... As in the nuclear rocket, the energy which propels the xenon jet comes from a different source; here it is electrical energy from solar cells. ... The XIPS ("zips") ion engine developed by the Hughes corporation was tested in the laboratory and then aboard a Russian spacecraft, launched 6 October 1997; it is the one shown on top of this page. ...

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• Prediction technique
• The Solar Wind
• The Brightest Moon

... It is found that the correlation coefficients between these two parameters calculated separately inside and outside the sunspot formation zone ±30 have cyclic variation and occur in anti-phase. This suggests different mechanisms of formation of the corona in the fields of small, medium, and large scales. ... The relationship between the coronal green line brightness (CGLB) and the magnetic field strength (MFS) has been investigated by constructing the corresponding synoptic maps for the 1977-2001. ...

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• IZMIRAN
• Chains and CMEs
• Heliophysical Laboratory of IZMIRAN (Solar-Terrestrial Physics Division)

Next: Strongly Interacting Galaxies Up: The Group of Nearby Previous: NGC 7552 . is a barred spiral which is interacting with several bright neighbours, namely NGC 7590, NGC 7599 (see Fig. 12), and most likely also NGC 7552 (see above). ... Figure: H I distribution (contours) of NGC 7582 and two nearby galaxies, NGC 7590 ( = 1596 kms -1 ) and NGC 7599 ( = 1654 kms -1 ) overlaid onto the optical emission (greyscale) from the Digitized Sky Survey (DSS). ...

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• NGC 1808
• ATNF Daily Astronomy Picture
• The HIPASS Bright Galaxy Survey

Astronotes Armagh Planetarium's Stellar Blog! ... Moon . Planets . ... Monthly Sky Notes . ... February . ... The ringed planet will be quite bright, but unlike Jupiter it will not be the brightest point of light in the sky, this accolade will return to Sirius which is the brightest star in our night sky in the constellation of Canis Major. ... Seven days later on February 18, the Moon will be in its full Moon phase. ... Tweets that mention Wonders of the February Night Sky | ... Astronotes . ...

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• stars | Astronotes - Part 6
• ESO | Astronotes - Part 3
• - Part 41