. " The Arecibo Observatory is sponsored by the National Science Foundation. Any opinions, findings and conclusions or recommendations . expressed in this publication are those of the author(s) and do not necessarily reflect the views of the National Science Foundation."

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• Molecular Lines in Starburst Galaxies
• Summer 2012 REU Project Abstracts National Astronomy and Ionosphere Center
• CORRELATOR BOARDS

Next: The Model Up: No Title Previous: Radiopulsars as Sources of . In this section, we study the evolution of stellar populations on a time-scale of 10 Myr for a starburst љ occurring under conditions similar to those in the Galactic Center (see Lipunov et al. (1995d)[ 126 ]). We estimate the expected number of X-ray transient љ sources (NS + MS star), super accreting BH, and BH + supergiant binaries, all as functions of time elapsed after the burst. ...

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• Number of accreting X-ray binaries of selected types
• Gravitational Wave Background from Individual Galaxies
• AXAF web sites

... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Parkes | ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... The first claim that HI could be associated with a dSph-like system was for the dIrr/dSph system Phoenix (Carignan, Demers & CУДtУ? ...

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• Using CASA CentralProcessor 0.11 documentation
• ATNF Media Releases (1998)
• HIPASS Bright Galaxy Catalog

... The absolute magnitude of the RCBs in the LMC and the small number of Galactic RCBs implies that they are very rare stars. Together with statistics for related stars, the total number of hydrogen-deficient stars in the Galaxy is estimated to be about 1000. Whilst the luminosity of RCBs is similar to that of other low-mass stars as they evolve rapidly from the asymptotic RED GIANT branch to become WHITE DWARFS , their frequency is much lower. ...

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• Performance
• Armagh Observatory
• Research Activity and Funding Trends

Session 9 - The Hubble Deep Field. ... The Hubble Deep Field (HDF) experiment is a unique project to explore at unprecedented depth and angular resolution the faintest and most distant galaxies. ... This allows study of broad-band spectral energy distribution, morphology and number count statistics for galaxies that span the largest, if not the whole, time interval of galaxy history. ... Here we present preliminary number counts, color-magnitude and color-color diagrams for the 4 HDF frames. ...

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• HST this week: 049
• Gregory F Snyder
• Stellar Photometry

... Contacts . 2010: . Traces of recent interactions in active isolated galaxies . ... It is shown that in a sample of active isolated galaxies about 35% have undergone a merger with another galaxy during the last 0.5-1 billion years. ... Contacts: A.V.Moiseev ) . Posted: MNRAS, vol.408, p.400, 2010. ... A steeper drop was detected in the electron energy distribution for the GPS-galaxies, rather than for the GPS-quasars - the difference of the exponent is of about 0.46. ... Archive . ...

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• UGC 2172, NGC 3239
• Lack of Dwarf Galaxies in the Local Volume Compared to Conventional Cosmology
• Multi-Spin Galaxies Conference 2016

Next: Participants Up: Contents Previous: Cover This volume contains the papers presented at the fourth annual conference on Astronomical Data Analysis Software and Systems (ADASS IV) which was held at the Omni Inner Harbor Hotel in Baltimore, Maryland, from the 26th through the 28th of October 1994. ... To help keep up with new trends in software as they relate to advances in astronomy, the ADASS conferences are organized around certain topics of current interest. ...

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• Access to Data Sources and the ESO SkyCat Tool
• ADASS 2003 Conference Proceedings
• EMSAO: Radial Velocities from Emission Lines in Spectra

Next: First results from follow-up Up: Results of the NOT Previous: Results of the NOT . The HSS (Hamburg/SAO survey) constitutes a large collaborative effort between investigators of several countries (Germany, Russia, Ukraine, Israel, France and Spain) to produce a new, large and deep sample of blue compact galaxies in the sky area R.A.=7h20m to 17h40m, DEC=+35 to +50. Emission Line Galaxies (ELGs) are being selected using the plates from the Hamburg Quasar Survey (Ugryumov et al. ...

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• Classification criteria
• Catalog of Galaxies behind the Milky Way
• HyperLEDA documentation: parameter: pgc

... CXC , NASA Explanation: What do you call a group of black holes ... a flock, a brace, a swarm? Monitoring a region around the center of our Galaxy , astronomers have indeed found evidence for a surprisingly large number of variable x-ray sources - likely black holes or neutron stars in binary star systems - swarming around the Milky Way's own central supermassive black hole. ... Publications with keywords: galaxy center - black hole - x-ray binary - Sgr A . ... Jumbled Galaxy Centaurus A . ...

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• Twisting with NGC 3718
• Extra Galaxies
• Астронет > Extra Galaxies

Next: *tabplot* - Displaying a Up: Radial Profiles and Projections Previous: Radial Profiles and Projections . Obtain a radial distribution of counts for the source centered at x = 503, y = 513, in the data image xdata$snr.qp . The background is taken locally from an annulus outside the source region. ... Region descriptors can also be given on the command line, but they must be enclosed by quotes. xs> imcnts xdata$snr ``a 503 513 0 50 n=5'' . ...

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• Fit a source with a small number of net counts
• High Energy Astrophysics
• The Chandra Multiwavelength Project (ChaMP)

home membership . SEARCH ASP SITE: Match ALL words Match ANY word . General/ Technical Membership Form for new members . Renewal General/ Technical Membership Form . Gift Membership Form (New & Renewal) . Member Change of Contact Info . ... ASP E-mail Newsletters . ... Membership Number . ... Institution (leave blank if using home address) . Department (leave blank if using home address) . Street Address . ... New Phone . ... Previous Phone . ... home | ... membership | ...

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• ASP: An Ancient Universe - Overview
• ASP: Beacons in the Gloom
• ASP: What Have We Learned About Halley's Comet?

... This year SSAU provides 1429 state-funded places for admission in all kinds and directions of educational programs. ... In addition, SSAU Admission Committee notes the substantial increase in interest from the foreign applicants this year. The number of applications from foreign countries has already surpassed last year's totals - 76 applications. Based on the experience of admission campaigns of previous years, SSAU expects summer 2014 to enrol about 150 foreign students in the university. ...

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... The catalog contains SAO number; the right ascension and declination with a B1950.0 equinox and epoch; annual proper motion and its standard deviation, photographic and visual magnitudes; spectral type; references to sources; the Durchmusterung (DM) identifier if the star is listed in the Bonner DM (BD), Cordoba DM (CD), or Cape Photographic DM (CP); component identification; The Henry Draper (Extension) (HD or HDE) number; and J2000 positions and proper motions. ...

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• Uppsala General Catalogue of Galaxies

... The actual cross-correlations were done as follows: north of WGACAT was correlated with the GB6 catalog with a correlation radius of one arc minute. ... We therefore cross-correlated WGACAT with the GB6 and PMN radio catalogs with a 1.5 arcmin radius. ... As a result of this experiment, we then added to the WGACAT/PMN candidate list the 29 unclassified sources obtained from the 1.5 arcmin correlation and having PSPC offsets arcmin, ratio between X-ray/radio offset and positional error , and . ...

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• Number of papers published using different observatories | ESO
• Number of papers published using different observatories | ESO United States
• Number of papers published using different observatories | ESO Ireland

. Field of research interest . Cosmology, Active Galaxy Nuclei, gamma-bursts. Scientific Degree . PhD 1973 in Astropysics . Position . Head of Laboratory . Department Number . 01 (Theoretical Astrophysics) . Postal Address . Astro Space Center . of P.N.Lebedev Physical Institute . Russian Academy of Sciences . Profsoyuznaya St. 84/32 . Moscow, RUSSIA . Postal Code . 117810 . Telephone Number . +7(095) 333 3366 . FAX Number . +7(095) 333 2378 . E-mail . bkomberg@dpc.asc.rssi.ru

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• Illarionov Andrej Feodorovich, Astro Space Center (ASC)
• ASC home page
• Lukash Vladimir Nikolaevich, Astro Space Center (ASC)

... Department Number . ... Astro Space Center . ... Telephone Number . 7(495) 333 2523 . FAX Number . 7(495) 333 2378 . ... bkomberg@lukash.asc.rssi.ru . ...

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• Illarionov Andrej Feodorovich, Astro Space Center (ASC)
• Arkhipova Natalya Anatolievna, Astro Space Center (ASC)
• Malinovsky Alexandre Mikhailovich, Astro Space Center (ASC)

... Your main research interests lie in starburst galaxies. ... Perhaps it is the howling wind and lack of insulation in your offices that does it, but the glowing warmth of a galaxy violently forming vast numbers of stars has a great attraction to you. ... All the nearby galaxies that are forming stars at reasonable rates are very dusty: most of the radiation from their young stars and supernovae is absorbed by dust and re-radiated in the far-IR. ...

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• Dark Matter in Spiral Galaxies
• Designated Observatory Registry
• Signal-to-Noise Ratio

... 2008 July 17 . Extra Galaxies . ... The most striking is clearly NGC 3718 , the warped spiral galaxy right of center. ... A mere 150 thousand light-years to the left is another large spiral galaxy, NGC 3729. ... While this galaxy pair lies about 52 million light-years away, the remarkable Hickson Group 56 can also be seen clustered just below NGC 3718. Hickson Group 56 consists of five interacting galaxies and lies over 400 million light-years away. ... About APOD | ...

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• The Sparkle Plug-In: Features
• APOD Index - Galaxies: Milky Way
• The Sparkle Plug-In: The Sparkle Dialog Box

... Star Atlas . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... galaxies . stars . ... Globular cluster NGC 2808, elliptical galaxy NGC 2986, and the Sextans Dwarf . ... Discovery triples the number of stars in the universe . ... The hidden stars are known as red dwarfs for their color and small size. Because red dwarfs are small and dim compared to stars like the Sun, astronomers hadn't been able to detect them in galaxies beyond the Milky Way before now. ...

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• Could large numbers of black holes account for much of the "dark matter"
• The right number of images | Astronomy.com
• Super-sized galaxy | Astronomy.com

This service contributes to the International Service of Geomagnetic Indices (ISGI) of the IAGA . ... The Kp numbers of the previous month are available in tabular format . ... There are available also historical and current Kp and derived indices per anonoymos FTP (see below). ... U.S.A. FTP server: ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/ . monthly update) . ... contains the monthly Kp / ap tables in a simple text format readable for both humans and computers (*.tab). ...

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