Today's APOD | ... Editor's choices for the most educational Astronomy Pictures of the Day about our Milky Way Galaxy: . APOD: 2005 October 4 - The Milky Way in Stars and Dust . Explanation: The disk of our Milky Way Galaxy is home to hot nebulae, cold dust, and billions of stars. ... The thin disk of our home spiral galaxy is clearly apparent, with stars appearing white and interstellar dust appearing red. ... Explanation: Most bright stars in our Milky Way Galaxy reside in a disk. ...

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• APOD: 2015 April 19 - Ring Galaxy AM 0644 741 from Hubble
• APOD: 2011 April 5 - The Milky Way Over Tenerife
• APOD: 2008 April 25 - M86 in the Virgo Cluster

... Armagh Planetarium . ... Our Galaxy . ... Universe . ... For those of you that are still bearing the psychological scars from PlutoтАЩs demotion from planet to dwarf planet a decade ago, here is news that may add salt to [ ] . ... In 2015 Armagh PlanetariumтАЩs website (including Astronotes) received well over 2.6 million page views (and over 75 million web hits*) from all over the world. ... Here you will find the latest news and views from the fascinating worlds of astronomy and space exploration....

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• Finding Your Way in the Milky Way | Astronotes
• Astronotes | Armagh Planetarium's astronomy news from across the Universe -
• galaxies | Astronotes - Part 2

... 12.12.1996 . ... Credit: Andy Steere Explanation: There are more than a few stars in our Galaxy. ... In the northern hemisphere, away from city lights and during the summer months, part of the Milky Way can be seen behind the Summer Triangle of stars - Deneb , Vega , and Altair . ... Behind the Summer Triangle lies some of the vast star fields of our Milky Way Galaxy , containing literally billions of stars. ... Publications with keywords: Summer Triangle - Milky Way . ... A Milky Way Band . ...

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• M51: The Whirlpool Galaxy
• XWare > APOD

... Tonight's Sky . ... Sky this Month . ... space physics . ... The Sky This Week: April 1 - 10 . ... Sky this Week . ... Sky Events . Get to Know the Night Sky . Tour the Deep Sky . Sky Guide . ... Observing springtime deep-sky objects with a large telescope . ... Johns Hopkins University Applied Physics Lab, Laurel, Maryland . ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

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• Space: women neednт??t apply? | Astronomy.com
• Earth's laws still apply in distant universe | Astronomy.com
• What percent of star systems have orbits in the right orientation for

FOR RELEASE: August 7, 1996 PHOTO NO.: STScI-PRC96-27 GIANT STARBIRTH REGION IN NEIGHBORING GALAXY This is a Hubble Space Telescope image (right) of a vast nebula called NGC 604, which lies in the neighboring spiral galaxy M33, located 2.7 million light-years away in the constellation Triangulum. ... Image files in GIF and JPEG format and captions may be accessed on Internet via anonymous ftp from oposite.stsci.edu in /pubinfo. ...

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• APOD: 2000 April 4 - A Superwind from the Cigar Galaxy
• APOD: August 7, 1998 - M65 Without Moth
• APOD: April 12, 1999 - Nearby Spiral Galaxy NGC 4945

The Astronomical Society of Australia has been asked by STANDARDS AUSTRALIA to compile a list of "designated" optical observatories that are valuable resources for (i) research, (ii) education and (iii) community use. The ASA is the final arbiter of whether any particular observatory is so designated. ... Upon receipt of your application form, your observatory will be entered on a list of "Pending Designated Observatories" on the ASA Home Page. ... It will be emailed for you. ... Email . ...

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• Siding Spring Survey
• Dark Matter in Spiral Galaxies
• IAU Commission #34 (Interstellar Matter)

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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• The Galaxy Gallery Page 6: Comparative Morphology
• The Galaxy Gallery: Messier Objects
• Stellar and Galaxy Spectra

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... ATCA . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Powerful beams of relativistic plasma once emerged from a black hole in a galaxy located at the centre of this image and created the giant radio lobes that are 1.5 million light years in...

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• Evolutionary Paths in Galaxy Morphology
• Neutral Hydrogen Gas in the Circinus Galaxy
• Finding the Bivariate Brightness Distribution of galaxies from an HI selected

... A long time ago, in a galaxy far, far away, billions of stars shone brightly. ... In the photo you can see that the colour of the galaxy is different in the centre and the outer regions. The galaxy looks more yellow and orange towards the centre (astronomers say it is reddish ), while it is blue in the outer parts. ... But when you look up to the night sky, why do most of the stars look white, rather than a dazzling variety of colours? ... So we are only looking at these stars in black and white! ...

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• Los Cielos de Am , The darkest sky and the two galactic hemispheres
• Publications, Paul Bristow
• ESO - Science Announcements

The HST images of GRB 990510. The images were obtained on 8.1 June 1999 (UT), 17.9 June 1999 and 29 April 2000. ... On this page we present the Hubble Space Telescope images of GRB 990510. ... The field of GRB 990510 was imaged by HST on 8.1 June 1999 (UT) 17.9 June 1999 (UT) and 29 April 2000 with the STIS/CCD camera in Open Filter (50CCD) mode. ... The suggestion of a host in the June 1999 image, led us to re-image the field in April 2000. ... The 29 April 2000 image of the field of GRB 990510. ...

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• Abstract
• GRB 9900712
• Dr. Gilbert's Presentations

... Our recent observations with the Hubble Space Telescope (August 29, 2014) led to revealing a highly isolated dwarf spheroidal galaxy KKs 3 situated at a distance of 2.12 0.07 Mpc from the Milky Way. The dSph galaxy locates on the southern sky (RA=02 h 24 m 44.4 s , Dec.= ... Over the last decade, about 30 dSph galaxies have been discovered inside the Local Group through systematic search in the vicinity of M31 and more that a dozen dSphs were discovered in the nearby group around M81. ...

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• Large telescopes application form
• Galaxy sector, archive 2012
• Events archive

... Bad Astronomy . ... Bitesize Astronomy . ... Bad Astro Store . ... Slacker Astronomy . ... Keep Bad Astronomy close to your heart, and help make me filthy rich. ... Life Under the Moon . ... Seeing Jupiter's Moons . ... Time Zones and the Spherical Earth . A Companion to the Earth? ... December 19, 1999) . ... Big Moon, Little Moon . ... How Big is the Moon? ... 14, 2000) . ... 2008 Phil Plait. ... Subscribe to the Bad Astronomy Newsletter! Talk about Bad Astronomy on the BA Bulletin Board! ...

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• Phil Plait's Bad Astronomy: Q and BA
• Phil Plait's Bad Astronomy: Bad News

O ptimal transport : T heory and A pplications . ... This is a web site of the research project Optimal transport: Theory and applications to cosmological reconstruction and image processing (OTARIE) supported by the French National Research Agency ( Agence nationale de la recherche ) under contract ANR-07-BLAN-0235 . ... Optimal transport is a mathematical subject connecting the fields of optimization, partial differential equations, and dynamical systems in finite and infinite dimensions. ...

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• Conference "Arithmetic Geometry: Explicit Methods and Applications"
• How to get to "U Nikitskikh Vorot" theatre

... The Large Magellanic Cloud is a Dwarf Irregular galaxy in orbit around our own Milky Way. It is a large object, several degrees in size, and easily visible to the unaided eye in Southern Hemisphere skies. The LMC is located in the constellation of Doradus at about 5h30m Right Ascension, -68 degrees Declination, and lies at a distance of roughly 50 kiloparsecs (160,000 light years) from Earth. ...

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• The Pleiades
• REU Application Instructions
• HIPASS Results and Lessons

... Dept. for Physics of Stars&Galaxies . Dept. for Space Plasma Physics . Dept. for Physics of Minor Celestial Bodies . Dept. for Physics of Planetary Systems . Dept. for Solar Physics . Department for Atmospheric Optics . ... Kinematics&Physics.. ... 2016,MNRAS, Vol.455 ,is.1,p.357-369. ... 2016,MNRAS, Vol.456 ,is.1,p.181-191. ... 2016,ApJ, Vol.816 ,is.1,p.3. ... Applied Optics . ... Solar Physics . ... All Pages . ... N1-12 . ... microfish . ... Applied Spectroscopy (microfishes) . ...

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• MAO NASU :: Topic: Invitation to submit to Remote Sensing Applications: Society
• Publications
• Applied Optics - Стор?нка 2

... 13th European VLBI Network Symposium . and Users Meeting . on September 20-23, 2016. ... 13th European VLBI Network Symposium and Users Meeting on September 20-23, 2016. ... Year book "Ephemerides of Minor Planets for 2016" on-line . ...

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• EVN Symposium 2016
• KBHO-2013 first ann
• NAA 2011-2012 (preface)

... The bright supernova (hereafter SN) in the galaxy NGC 4527 was first sighted by S. Knight (USA) on April 13.17UT at magnitude ~14.0v. The report of the sighting was subsequently forwarded by phone to the AAVSO. ... SN 1991T. The galaxy NGC 4527 is an Sb(s)II type galaxy with an apparent Blue magnitude of 11.32 (Shapley-Ames, 1981). ... An analysis of this event utilizing visual observations by amateurs, plus a light curve is presented.. ... THE LIGHT CURVE: . ... ISN SN 1991T web page . ...

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• SN1989B in M66

Semiconductor Home > Products > Mixed Signal and Analog > CCD IMAGERS Family > . TC213, 1024- X 512-PIXEL CCD IMAGE SENSOR . ... The TC213 is a frame-transfer charge-coupled device (CCD) image sensor that provides very high-resolution image acquisition for image-processing applications such as robotic vision, medical X-ray analysis, and metrology. The image format measures 12.00 mm horizontally by 6.12 mm vertically; the image-area diagonal is 13.5 mm. ... 13.5-mm Image-Area Diagonal . ...

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• Emission-line galaxies
• "Structure" publications for 1997 year
• Catalogue of Principal Galaxies (PGC)

... Positive iterative deconvolution is an algorithm that applies non-linear constraints, conserves energy, and delivers stable results at high noise-levels. This is also true for Richardson-Lucy like algorithms which follow a statistical approach to the deconvolution problem. ... All algorithms resolve the objects, as shown by the reconstructions by Richardson-Lucy in Figure 2 on the right, the algorithm by M?ller in Figure 3 on the left and positive iterative deconvolution in Figure 3 on the right. ...

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• The Co-Addition Technique Applied to Images of Galaxy Cores
• Demonstration of Parallel AIPS++ Deconvolution Application
• Applications

... Also, let a, b and c be the lengths of its three sides-- a of the side across from A, b of the one across from B, and c the longest one, across from C. Two useful ratios associated with the angle A ("trigonometric functions of A ") are . The sine of A sin A = a/c (involving the side a across from A ) . The cosine of A cos A = b/c (involving the side b besides A ) . ... The tangent of A . ... Calculators usually have a button " tan " which, if you punch in the angle, gives you the tangent. ...

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• (S-7a) The Black Hole at the Center of our Galaxy
• Applying Kepler's Third Law