M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...

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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Risks Comparable to NEOs . ... The Increasing Rate of Discovery of Asteroids . ... Comet and Asteroid Collision Probabilities . ... Extreme albedo comets and the impact hazard (PDF Format) . ... Asteroid Impact Animations . ... Workshop on Scientific Requirements for Mitigation of Hazardous Comets and Asteroids - 2002 . ... The Spaceguard Survey Report, 1992 (PDF) . Tsunami from Asteroid/Comet Impacts . ...

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• Las Cumbres Observatory, Asteroids, comets, Messier objects, supernova

... Each point shows the 1 sigma photometric errors and the time span covered by the data; the dotted lines are the 3 sigma limits of each image. ... The solid thick lines are a fit obtained from a K-corrected, time-dilated SNIb light curve at z= 0.95 with tmax=34.0, E(B-V)=0.04 and omega=0.1. ... The three images on the left are the total HDF-N images by Williams et al. 1996 with a pixel scale of 0.04 arcsec/pixel. ... Each image is labelled by the filter and the time range of the observations in days....

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• K-band Arcetri Obscured Supernova Search - Detected Supernovae
• Star formation
• The relationship between NSs and SNRs (Elba, June 1-4,1998)

... Supernova 1987A in the Large Magellanic Cloud presents unprecedented opportunity to observe the evolution of a supernova at all wavelengths. While optical observations with the HST Faint Object Camera have obtained resolutions of 0."1, we are limited in the radio to the resolution obtainable with the Australia Telescope Compact Array (ATCA). ... At this resolution the radio supernova is distinct from a point source, but few physical conclusions can be drawn. ... Keywords: Superresolution, Radio . ...

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• Briggs: Comparative Deconvolution Study of SN 1987A
• Observing Faint Targets Near Bright Objects
• STIS Instrument Handbook

... The search for distant objects which can be both galaxies and quasars is one of the most important problems of observational astrphysics, because it allows one to determine cosmological parameters connected with the time of appearence and evolution of stellar systems, large scale structure of the Universe. ... Radio galaxies are important objects to be studied because they are sources of infrared-optical-ultraviolet continuum, emission lines and continual radio emission. ...

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• Laboratory of spectroscopy and photometry of extragalactic objects :MOUSER
• Emission molecular bands
• On the problem of high spectral resolution observations of faint objects

... Contacts . 2012: . ... We refined the fundamental parameters of the components, the orbital periods, and the conditions of photospheric heating of the secondary component by the ultraviolet radiation of the hot component. ... The observations of the star clusters associated with ultra-luminous x-ray sources (ULXs) in four galaxies on the 6-meter and VLT telescopes have shown that all the ULXs are located within 200pc of very young star clusters (younger than 5 million years). ... Archive . ...

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• Detection of unique bright radio flare of X-ray binary
• RCJ0311+0507
• Detection of Radio Transients and Variable Radio Sources Using the Archive Data

... Click on an object in the solar system or choose from the list at left to learn more . The Arecibo Observatory planetary radar is the world's most powerful instrument for post-discovery characterization and orbital refinement of near-Earth objects. ... The Solar System Studies group is a department of the Arecibo Observatory, which is an NSF facility operated under cooperative agreement by SRI International, Universities Space Research Association (USRA), and la Universidad Metropolitana (UMET). ...

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• What is a pulsar?
• THE SOURCE LIST

... Observing . ... Observing springtime deep-sky objects with a large telescope . Springtime observing for small telescopes . ... Astronomy magazine Editor David J. Eicher shares 10 of his favorite springtime deep-sky objects, including the NGC 3190 galaxy group, 3C 273, and NGC 3242. ... In this video, Astronomy magazine Editor David J. Eicher discusses deep-sky objects in the spring sky you can see with a 12-inch or larger telescope. ... Get instant access to subscriber content on Astronomy.com! ...

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• More spring objects to observe | Astronomy.com
• 50 Weirdest Objects in the Cosmos | Astronomy.com
• near earth objects | Astronomy.com

... Up: Data Analysis and Processing Techniques . ... Also, a method for quality control of CCD observations is suggested. ... Everyone who observes a celestial object using a CCD detects moving celestial objects as a ``by product''. ... We hope that our investigations may be useful for near-Earth space control and also for searches of the moving celestial objects through analysis of old and new CCD frames obtained at any amateur or professional astronomical observatory. ...

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• ETCs and Observations Simulation at the VLT
• Modeling Scattered Light in the HST Faint Object Spectrograph
• System Interfaces to the STIS Calibration Pipeline

X­RAY STUDY OF CRAB­LIKE AND COMPOSITE SNRS K. TORII, H. TSUNEMI Osaka University AND P. SLANE Harvard­Smithsonian Center for Astrophysics 1. ... We have observed several objects including 3C58, CTA1, and G292.0+1.8. ... 1997; Torii et al. 1997). ... Al­ though the center­filled radio morphology suggested an interior plerionic component, strong X­ray emission lines seemed to rule out such specula­ tions. ... G292.0+1.8 0.5 ­ 2 keV G292.0+1.8 2 ­ 10 keV Figure 1. ASCA SIS images of G292.0+1.8. ...

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• Very Low Mass PMS Objects
• Pat Slane: Pulsar Papers
• Chandra Images for SNR J0500.0-7007

... Galaxy Evolution home . ... Micro quasars Publications . ... In the last few years a very similar phenomenon has been observed in some X-ray binaries, binary stellar systems with one gravitationally-compact object (black hole or neutron star) and an "normal" star part of whos atmosphere is captured by the compact object. ... The compact objects (a few solar masses) are much smaller than those inferred in AGN (10 9 solar masses), and the sizes much smaller, so the analogy may not be complete. ...

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• Galaxy Evolution: Cosmological evolution of star formation
• Galaxy Evolution: Radio sources and their environments
• Astrophysics Group Pulsars

Next: Radiopulsars as Sources of Up: Cosmic Rays and Evolution Previous: Cosmic Rays and Evolution . Presently, there is little doubt that galactic CR can be generated at rapidly expanding shock fronts produced by supernova explosions. ... Statistical properties of radiopulsars in our Galaxy indicate a formation rate of NS of about 1 per 10-20 years in the present cosmological epoch, while direct astronomical observations have so far not detected supernova explosions at this high rate. ...

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• #tex2html_wrap_inline12480#-#tex2html_wrap_inline12482# Dependence for the
• X-ray Luminosity Evolution
• #tex2html_wrap_inline12527#-#tex2html_wrap_inline12529# for Supernova...

Stellarium 0.12.3 . ... Classes . ... Supernova Class Reference . ... Supernova (const QVariantMap &map) . ... Get a QVariantMap which describes the supernova. ... getSelectPriority (const StelCore *core) const . ... getInfoString (const StelCore *core, const InfoStringGroup &flags) const . ... getVMagnitude (const StelCore *core, bool withExtinction=false) const . ... getAngularSize (const StelCore *core) const . ... getPositionInfoString (const StelCore *core, const InfoStringGroup &flags) const . ...

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• Stellarium: Quasar Class Reference
• Stellarium: Nebula Class Reference

In 1950 Jan Oort noticed that . no comet has been observed with an orbit that indicates that it came from interstellar space, . ... From this he proposed that comets reside in a vast cloud at the outer reaches of the solar system. ... Unfortunately, since the individual comets are so small and at such large distances, we have no direct evidence about the Oort Cloud. ... Its orbit is intermediate between the Kuiper Belt and what was previously thought to be the inner part of the Oort Cloud. ...

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• Contributions by amateurs: SN1996X.
• SAI Supernova catalog
• Bilbio

... To separate stellar spectra from other non emission-line spectra we use a template with the most common stellar features which is cross-correlated with the observed spectra. ... The remaining stellar spectra are roughly classified as A - G stars, most of them having intermediate types between A and F, or F and G. The coordinates, apparent magnitudes, spectral types and lists of absorption features identified in the spectra of these objects are given in Table 5. root . 1998-11-24 ...

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• Results of follow-up spectroscopy
• Emission-line galaxies
• The Hamburg/SAO Survey for Emission-Line Galaxies

Pulkovo NEO Page . ... EPOS Software Package . ... EPOS ( E phemeris P rogram for O bjects of the S olar system) is the Windows PC application for study and ephemeris support of observations of the Solar system objects. ... It controls the part of common data and transfers the control to one of the programs that solve the restricted set of tasks. ... So with the EPOS software package one can calculate the accurate ephemerides for many objects and get the quick illustration of their motion as well. ...

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• Pulkovo NEO Page: Estimation of Accuracy of the Observations

Supernova 2002an in NGC 2575 . This page is devoted to information on Supernova 2002an in NGC 2575 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. Discovered by Japanese amateur Yasuo Sano . ... Yasuo Sano's 2002an discovery page . ... Image Credit . ... Mag . ... 2002/01/22.522 . ... Yasuo Sano image . ...

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• Supernova 1999dh in IC 211
• Bright Supernova pages - Statistics for 2002
• Supernova 2011ht in UGC 5460

... Public . Science . ... Science Users Information > Science Publications > Science Announcements . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... Data Handling and Products . ... Science Data Products Forum . ... ESO Data . ... Science Announcements . ... Published: 17 Sep 2014 . An extended set of FAQs (Frequently Asked Questions) on data reduction is available . ... Published: 28 Aug 2014 . ... This feature is available for all ALMA programmes, except for science verification data. ...

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• Identifications and Efficiency
• ESO - Thesis Topic: Evolution of SN 1987A
• ESO - Is it possible to calibrate the visibility data of our object with a

STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . LX850 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Coronado€о Solar . ... Spotting Scopes . ...

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• Telescopes - Products
• Products

... 1987) MM observations of pre-planetary disks · Methods ­ Millimetre single dish ( Mopra ) and interferometric (ATCA) spectral line and continuum observations , to obtain gas chemistry, kinematics (infall, outflow, rotation), gas and cold dust spatial distribution ­ Mid - infrared spectroscopic observations of the 10, 20 micron silicate bands (Michelle on UKIRT/Gemini-N, TIMMI2 on ESO 3.6 m, T-ReCS on Gemini-S), to obtain warm ... Mopra observations of HD 163296 Grady et al. ...

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• http://www.atnf.csiro.au/observers/apply/ATCA_legacy_EOI_apopping.pdf
• Searching For Supernova Remnants
• SN 1987A