... Tentacles of the Tarantula Nebula . ... Credit Copyright: WFI , MPG/ESO 2.2-m Telescope , La Silla , ESO Explanation: The Tarantula Nebula is a giant emission nebula within our neighboring galaxy the Large Magellanic Cloud . ... The Tarantula Nebula , also dubbed 30 Doradus, lies 170,000 light years away toward the constellation of Dorado . ... Publications with keywords: Tarantula Nebula - LMC - 30 Doradus . Publications with words: Tarantula Nebula - LMC - 30 Doradus . ... Hydrogen in the LMC . ...

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• R136: The Massive Stars of 30 Doradus
• Star Cluster R136 Bursts Out
• Massive Stars Of 30 Doradus

... 2004 December 28 . Tentacles of the Tarantula Nebula . ... The energetic light and winds from this cluster light up the nebula and sculpt the surrounding gas and dust into vast complex filaments . These "tentacles" give the Tarantula Nebula its name. ... A 300 light-year portion of the Tarantula Nebula is imaged. The Tarantula Nebula , also dubbed 30 Doradus, lies 170,000 light years away toward the constellation of Dorado . ... About APOD | ... NASA Official: Jay Norris. ...

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• APOD: 2005 December 11 - R136: The Massive Stars of 30 Doradus
• APOD: 2008 December 1 - Massive Stars Resolved in the Carina Nebula
• APOD: 2014 December 9 - The Flame Nebula in Visible and Infrared

... 2000, ApJ, 537, L49 . ... F. Palla . Invited Talk at the IAU Symposium 200 "The formation of binary stars" eds. R.D. Mathieu and H. Zinnecker (ASP Conf. Ser.) in press . Optical follow-up of ROSAT discovered candidate members of the open cluster Coma Berenices . ... 2000, A , in press . ... 2000, ApJ, in press . ... 2000, ApJ, in press (Sept. ... 2000, ApJ Lett., in press . ... Click to examine publications from other years . ... Star Formation Group . ... Arcetri Home Page . ...

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• FIRST LIGHT OF ARNICA AT TNG
• APOD: July 13, 1999 - The Flame Nebula in Infrared

... GSAOI Home . ... Science . ... Deep imaging at J , H , and K is required to identify all stellar objects, brown dwarfs, and planetary mass objects in the central region of the Orion Nebula Cluster down to masses comparable to that of Jupiter. This is required to establish the initial mass function, i.e., the number of stars of each mass that have formed, in this region of intense massive star formation. ... The fields of the GSAOI detectors are shown as four green squares in each frame. ...

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• IAU Commission #34 (Interstellar Matter)
• Julie Banfield | Astronomer
• GSAOI Globular Cluster Science Page

home publications > mercury . ... Big Clusters, Tiny Galaxies . ... Astronomers struggle to understand why giant star clusters form in the tiniest of galaxies . ... These clusters are probably young versions of globular clusters, but they are commonly called super star clusters. Seven dwarf galaxies within 16 million light-years have formed super star clusters, with one of these galaxies, NGC 1569, possessing two young clusters. ... Super star clusters have a lot to tell us about star formation. ...

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• ASP: Exploring Invisible Skies

... Australia Telescope Compact Array . ... Compact Stellar Systems in the Fornax Cluster: Super-massive Star Clusters or Extremely Compact Dwarf Galaxies? ... We suggest that these objects are either super-massive star clusters (intra-cluster globular clusters or tidally stripped nuclei of dwarf galaxies) or a new type of low-luminosity compact elliptical dwarf (``M32-type'') galaxy. ... Keywords: galaxies: star clusters -- galaxies: dwarf -- galaxies: formation . ... Properties of the compact objects ...

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• Evolutionary Paths in Galaxy Morphology
• ATNF Colloquium
• ATNF Science Highlights

Photon Scattering: Basic Principle of Photon Scattering . Audio Narration is available . No Scattering: Photon Source and Detector . ... For optical photons, scattering goes as wavelength to the -4 power. In the case of blue photons compared to red photons, this means that blue photons are about 10 times more likely to get scattered than red photons. ... Watch the blue photons scatter away from the detector . ... Interstellar dust make stars appear redder than they really are . ...

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• Astronomy HyperText Book: Stellar Clusters
• Constrains on Dark Matter
• Cosmological Issues for Theorists

Program number . ... Infrared Snapshots of 3CR Radio Galaxies . Abstract . ... Holland Ford, The Johns Hopkins University . ... An ACS H-alpha Survey of the Carina Nebula . ... A Snapshot Survey of the most massive clusters of galaxies . ... An ACS Imaging Survey of the Galaxies Hosting Strong Mg II Absorption . ... ACS observations of the galaxies in a giant Ly-alpha nebula at z~2.7 . ... An ACS Survey of a Complete Sample of Luminous Infrared Galaxies in the Local Universe . ... Past weeks: . ...

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• HST this week: 343
• Dr. Laura Watkins
• CLASH: An Innovative Survey to Place New Constraints on the Fundamental

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Dynamical models of multiple globular cluster populations around massive galaxies . ... Different techniques have been devised to separate multiple GC populations and perform dynamical analyses. ... Within this project, the PhD candidate will examine mock models of multiple GC populations around massive galaxies, devising `blinded' functional tests and comparing the possible sources of bias in different techniques....

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• Infrared/visible-light comparison of the Carina Nebula | ESO
• ESO - star07
• Infrared/visible-light comparison of the Carina Nebula | ESO Australia

Astronotes Armagh Planetarium's Stellar Blog! ... Milky Way . Stars . ... This dramatic image depicts Omega Centauri, one of 200 or so globular clusters orbiting our Milky Way galaxy. ... Swarms of tightly packed stars, numbering in the thousands to low millions, globular clusters are cosmic fossils, relics of the early times of our galaxy. Omega Centauri may actually be the core of a smaller galaxy ripped apart and assimilated by our own Milky Way in the distant past. ...

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• Our Galaxy | Astronotes - Part 5
• Astronotes | Armagh Planetarium's astronomy news from across the Universe -
• stellar nursery | Astronotes

... The most powerful and widely used methods to calculate the scattering matrix of a fractal cluster are based on the coupled dipoles methods (e.g. the Discrete Dipole Approximation, DDA) and the theory of light scattering by a cluster of spherical particles [2-4]. ... At present the procedure of calculation of the scattering matrix is well developed for both an oriented cluster of spherical particles and for chaotically oriented clusters of such particles [4]. ...

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• INTAS project 2003
• INTAS project 99/652: Publications

... Kopylov, A.I., Kopylova, F.G. "Structure of galaxy groups and clusters and measurement of their masses", . ... Kopylova, F.G., Kopylov, A.I. "Peculiar motions of galaxy clusters and groups in the Hercules and Leo supercluster regions", . ... Kopylova, F.G., Kopylov, A.I. "Analysis of the properties of clusters of galaxies in the region of the Leo supercluster", . ... Kopylova, F.G., Kopylov, A.I. "Analysis of the properties of clusters of galaxies in the region of the Ursa Major supercluster", . ...

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• Galaxy sector, archive 2012
• Galaxy sector, archive 2007
• New LBV Discovered in DDO 68 Galaxy

... The Pleiades star cluster, also known as the Seven Sisters and Messier 45, is a conspicuous object in the night sky with a prominent place in ancient mythology . ... The stars in the Pleiades are thought to have formed together around 100 million years ago, making them 1/50th the age of our sun, and they lie some 130 parsecs (425 light years ) away. ... Data for these stars are listed in a table below. ... Yes . ... WEBDA Pleiades cluster data . ... M45: The Pleiades Star Cluster (2007 November 18) ...

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• Pulsar Highlights - A Dozen new MSPs in Globular Clusters
• The Tarantula Nebula
• What is HISA?

... On the nature of the bi-stability jump in the winds of early-type stars Vink, J.S., de Koter, A., Lamers, H.J.G.L.M. 1999, A&A, 350, 181 3. ... New theoretical mass-loss rates of O and B stars Vink, J.S., de Koter, A., Lamers, H.J.G.L.M. 2000, A&A, 362, 295 5. ... Spectroscopic Dating of Very Massive Stars de Koter, A., Vink, J.S., Lamers, H.J.G.L.M. 1999, in: Spectrophotometric Dating of Stars and Galaxies, eds. I. Hubeny, S.R. Heap, R. Cornett, ASP Conf. ... Are all young stars disc accretors? ...

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• Armagh Observatory
• Stars Beyond Maturity
• Jorick Vink

... If all photons have the same speed (the speed of light) and the same mass (zero), why does an individual gamma-ray photon have more energy than a radio-wave photon? ... The equation E=mc 2 states that mass ( m ) and energy ( E ) are manifestations of the same thing; mass can change into energy, and energy can change into mass. The speed of light ( c ) is the conversion factor between the two quantities. ... Get instant access to subscriber content on Astronomy.com! ...

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• Bright planets meet at dusk | Astronomy.com
• Chandra weighs most massive galaxy cluster in distant universe | Astronomy.com
• New class of gravitational lenses | Astronomy.com

... Phase light curves of binary model that consists of a primary component with mass M 1 and a secondary component with mass M 2 . ... The input parameters of the problem are the accretion rate onto the binary components ( ), the component mass ratio q = M 2 /M 1 , the orbital inclination to the line of sight , the eccentricity e, the rotation angle of the apsidal line relative to the observer , and the parameter c characterizing viscosity. ...

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... Image Quality of the VLT . Total Optical Control . First light for the ESO VLT unit telescope 1 occurred during the workshop. ... The image shown (Figure 1 ) here was obtained with the VLT on May 16, 1998, in red light (R band), i.e. while the mirror was still uncoated. ... In this diagram (FIgure 2), the measured image quality of the VLT UT1 astronomical images is plotted versus the ``seeing", as measured by the Seeing Monitor, a small telescope also located on top of the Paranal Mountain. ...

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• ESLAB 2007

... Abubekerov M.K., Lipunov V.M. "The Lower Temperature Limits Of Accretors" Astronomy Reports, 2003, Vol. 47, Issue 8, pp.679-684. ... Abubekerov M.K., Antokhina E.A., Cherepashchuk A.M. "The Masses of X-ray Pulsars in Binary systems with OB Supergiants" Astronomy Reports, 2004, Vol. ... Abubekerov M.K., Antokhina E.A., Cherepashchuk A.M., Shimanskii V.V. "The Mass of the Compact Object in the Low-Mass X-ray Binary 2S 0921-630" Astronomy Reports Astronomy Reports, 2006, Vol.50, Issue 7, pp.544-552. ...

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• Yuri Nicolaevich Efremov - My Home Page

... Astrophysics Group . ... AMI Science . ... Observations of galaxy clusters are central to the AMI science programme. The AMI Small Array is used to observe already-known clusters with high-sensitivity and resolution, allowing us to extract detailed information about individual clusters and to build up statistics about the cluster population. ... Observing galaxy clusters at 15 GHz is tricky because of the contamination from foreground radio sources, which is where the Large Array comes in! ...

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• Martin Krause - Publications
• The history of star formation and mass assembly in early-type galaxies
• Astrophysics Group AMI Publications

Our early publications since 1990 till 1995 year . ... 7.Yu.I.Izotov, N.G.Guseva, V.A.Lipovetsky, A.Yu.Kniazev, J.A. Stepanian, 1990, Nature, 343, 238, Unusual low heavy-element abundance found in the blue compact galaxy SBS 0335-052 8.Yu.I.Izotov, N.G.Guseva, V.A.Lipovetsky, A.Yu,Kniazev, J.A.Stepanian, 1990, Physical Processes in Fragmentation and Star Formation, 1990, Kluwer Academic Publisher, p.235-240. ... New blue compact dwarf galaxies with low heavy-element abundances. ... 1993. ...

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• THE TEXAS SURVEY: Optical identifications
• "Structure" publications in 1996 year
• "Structure" publications in 2008 year