Astronomy Picture of the Day . ... Unusual Clouds over Hong Kong . ... NGC 3310: A Starburst Spiral Galaxy . ... Roughly 100 million years ago, NGC 3310 likely collided with a smaller galaxy causing the large spiral galaxy to light up with a tremendous burst of star formation. ... IC 1848: The Soul Nebula . ... The Tarantula Nebula is more than a thousand light-years in diameter, a giant star forming region within nearby satellite galaxy the Large Magellanic Cloud, about 180 thousand light-years away. ...

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Dust emission from the Type II supernova SN 2002hh in NGC 6946 has been detected at mid-infrared wavelengths by the Spitzer Space Telescope from 590 to 758 days after outburst and confirmed by higher angular resolution Gemini North mid-IR observations. ... The minimum emitting radius of 1.1У?1017 cm is too large for the emitting dust to have been formed in the supernova ejecta. ... ADS Citation Query . citations = 25 . ... 2006,6][2007,4][2008,2][2009,4][2010,2][2011,3][2012,1][2013,2][2015,1] . ...

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• The Incidence of Highly Obscured Star-forming Regions in SINGS Galaxies
• The Herschel revolution: Unveiling the morphology of the high-mass
• brown dwarfs - 1

... High-velocity clouds (HVCs) were discovered by Muller, Oort & Raimond (1963) in the 21-cm line emission of neutral, atomic hydrogen. They are gas clouds which are characterised by high radial velocities incompatible with a participation in the rotation of our Galaxy. ... This suggestion was seized by Braun & Burton (1999) who identified 66 compact high-velocity clouds (CHVCs) with positional and kinematic characteristics being compatible with a distribution across the entire Local Group. ...

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• Research - All-sky map of high-velocity clouds
• ATNF Daily Astronomy Picture
• Molecular gas

... 2016 February 23 . A Supernova through Galaxy Dust . Image Credit: NASA , ESA , and the Hubble Heritage ( STScI / AURA ); . Inset Image: Howard Hedlund Dave Jurasevich , Las Campanas Obs. Explanation: Telescopes around the world are tracking a bright supernova that occurred in a nearby dusty galaxy. ... Cen A is featured here in a high-resolution archival Hubble Space Telescope image, with an inset image featuring the supernova taken from the ground only two days after discovery. ...

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• APOD: 2016 February 25 - Highest, Tallest, and Closest to the Stars
• APOD: 2016 February 26 - The Tarantula Nebula
• APOD: 2001 February 16 - Star Forming Region Hubble X

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: High-Contrast Imaging of Planet-Forming Disks in Intermediate-Mass Young Stars . ... ESO-MIDAS . ... ESO HST Image Galleries . ... history, and the different processes that act to dissipate the disks around young stars from which these planets have formed. Using recently obtained data with SPHERE, the new high-contrast imaging facility at ESO's Very Large Telescope, the PhD project . ... intermediate-mass stars. ...

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• ESO - Circumstellar Dynamics at High Resolution
• High-Resolution Spectrum of the Ant Planetary Nebula around 12.8ѕ®m | ESO
• High-Resolution Spectrum of G333.6-0.2 around 12.8ѕ®m | ESO

National Aeronautics and Space Administration . ... Bruce McCandless II (Captain, USN, Ret.) NASA Astronaut (former) . ... He was a member of the astronaut support crew for the Apollo 14 mission and was backup pilot for the first manned Skylab mission (SL-1/SL-2). ... A veteran of two space flights, McCandless has logged over 312 hours in space, including 4 hours of MMU flight time. ... With the completion of this flight McCandless logged 191 hours in space (including 4 hours of MMU flight time). ...

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• Astronaut Bio: Stephen G. Bowen (2/2013)
• Astronaut Bio: Mark C. Lee 10/2006
• Astronaut Bio: Clayton C. Anderson (01/2013)

... 2010, A , in press . SiO outflows in high-mass star forming regions: A potential chemical clock? A. Lopez-Sepulcre, C.M. Walmsley, R. Cesaroni, C. Codella, F. Schuller, L. Bronfman, S.J. Carey, K. M. Menten, S. Molinari, A. Noriega-Crespo . ... A comparative study of high-mass cluster forming clumps . ... Class I and Class II methanol masers in high-mass star forming regions . ... Click to examine publications from other years . ... Star Formation Group . ... Arcetri Home Page . ...

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• High-resolution Herschel spectroscopy reveals the proto-planetary disk around
• A Search for Clustering around Herbig Ae/Be Stars
• High energy

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... It turns out one possibility is a form of matter/energy invented by Einstein in the 1920s to make sure his equations of General Relativity did not predict the Expansion of the Universe. Although Einstein was willing to predict several things with his equations of General Relativity, he obviously thought an expanding Universe was too much, and so he invented the Cosmological Constant, which repels itself, and was meant to balance the force of gravity, and make the Universe static. ...

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• Siding Spring Observatory's 2.3 m telescope (wide and high vantage point)
• Designated Observatory Application
• High Energy Astrophysics

.

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• U of O High Energy Physics Seminars
• University of Oregon Center for High Energy Physics - Public Lectures

. -!> download . Left: Consequtive explosion of 20 supernovae during 30 Myr. Right: Single hypernova (GRB) explosion with the total energy equivalent to 20 supernovae. The simulation was performed using a 2D Eulerian hydro code. The animation was done using IDL. -!>

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... Observatory tours are usually conducted by the Librarian, who in 2000 showed approximately 500 individuals from 19 different countries around the Observatory. These figures highlight the success of the Armagh Observatory's `open door' policy to attract visits by interested members of the public, groups and societies. ... In addition to tours, the Observatory also organized several public lectures, and hosted a number of special events during 2000. ...

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• High-Mass Star Formation
• Armagh Observatory
• Sakurai?s Object (V4334 Sagittarii)

2014 May version . ... Green D. A., 2014 , Bulletin of the Astronomical Society of India, 42 , 47-58. ( .pdf , or arXiv.org:1409.0637 ) If you make use of the detailed version of the catalogue, then plaese also cite: . Green D. A., 2014, `A Catalogue of Galactic Supernova Remnants (2014 May version)' , Cavendish Laboratory, Cambridge, United Kingdom (available at "http://www.mrao.cam.ac.uk/surveys/snrs/" ). ... Copyright D. A. Green 2014. 25872nd access to this version of the catalogue. ...

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• Bojan Nikolic -- 90 GHz Continuum Observations of Messier 66
• Research | Matt Bothwell
• Astrophysics Group Astrophysics Admissions Form

... The ESO-MIDAS Problem Report Form is the on-line user support service for reporting problems, questions and comments. Please fill out the form and send it off by clicking the SUBMIT button at the bottom of this page. However, before submitting your problem report it may be useful to check if is not already included in our Frequently Asked Questions page. support . ... Graphical User Interfaces . ... Sent comments on this screen to ESO-MIDAS < midas@eso.org > . ...

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• A Sample of 669 Ultra Steep Spectrum Radio Sources
• SNRs Spectra Request Form
• RMT_HOME_PAGE

... For the past years I have been working on the problem of synthesis of light curves of close binary systems, consisting of a normal star and a compact object (point object with fixed X-ray luminosity). ... Possible existence of a bright spot on the disk's lateral surface is taken into account. ... The last of then will be published in Gordon and Breach Publishers ( Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ... Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Yu. ...

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• Eugene Trunkovsky

... Team . ... V.V.Sokolov "The gamma-ray bursts, core-collapse supernovae and global star forming rate at large redshifts" . ... I.V.Sokolov, A.S.Moskvitin, Eda Sonbas, O.V.Verkhodanov, O.P.Zhelenkova "A galaxy cluster in the GRB 021004 field" . ... The monitoring of GRB afterglows and the study of their host galaxies with the SAO RAS 6-m telescope from 1997". ... A.S.Moskvitin, T.A.Fatkhullin, V.V.Sokolov and V.N.Komarova, "Spectral and photometric monitoring of CCSNe at SAO RAS" . ...

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• Results scientific researchs LRS
• High-resolution Near-infrared Study of the Deeply Embedded Young Stellar Object
• GOS home page

. Family name : . First name : . Second name : . Scientific degree : . Affiliation (in full) : . Affiliation (short form for badge) : . Affiliation (short form for badge) . Postal address : . Phone : . Fax : . E-mail : . Title of paper . Co-authors : . Type of presentation : . Oral Poster . To previous page . To first page

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• AKO-2005

... RAS members working in ISSP . ... The Institute of Solid State Physics (ISSP) was formed by the USSR Academy of Sciences on February 15, 1963, with a view to realize an efficient combination and interaction between fundamental research in condensed matter physics and materials science. ... Main Directions of Scientific Research Institute of Solid State Physics RAS (ISSP RAS) . ... Address: Institute of Solid State Physics RAS, Chernogolovka, Moscow District, 2 Academician Ossipyan str., ...

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• International Astronomy Olympiad: Form for the short report of National
• LHPP ISSP RAS
• II-VI compound crystal growth, HPVB & HPVZM basics

Halo around the Moon. Halo arises when the light beams refracted on the high clouds icy chips ina form of a six side prism. As a result we see a small halo circle with a 22°-radius. The big circle is formed by the beams paased through the side edge and the base of prismochips. Its radius is equal to 46° (nearly). The big circle is observed rarely and is shining weaker but it is easier to observe it near the Sun, if comparing with the small halo invisible in the bright Sun light. ...

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• plazmae

. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

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