... The dayside auroral precipitation consist of magnetosheath related boundary layer precipitation, and plasma sheet related BPS/CPS precipitation (extensions of the nightside precipitation regions). ... For example, the much lower fluxes from the LLBL region when compared to the cusp are compensated by the bidirectional electron beams found in the LLBL: the precipitating energy fluxes in the LLBL and the cusp are not that different. ... directly through the cusp and plasma mantle . ...

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... 2001) MIR detection rate towards water masers: ~80% (De Buizer et al. ... Is accompanied by outflow Surprisingly, near-IR outflow observations in H2 showed emission PARALLEL to maser distributions, not perpendicular De Buizer (2003) surveyed sites of linearly distributed methanol masers at CTIO ґ ONLY 2 had emission perpendicular to the maser distribution ґ 12 (86%) had emission parallel to the maser distribution De Buizer (2003) G319.95-0.20 G320.23-0.28 Surprisingly, near...

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• ATCA_mm_science
• ATNF Colloquium
• The Peculiar Spiral Galaxy NGC 1808

Neutral hydrogen distribution in the region of radio source Cygnus X . ... HI distribution in the region of radio source Cygnus X and supernova remnant G78.2+2.1 has been investigated from observations in 21 cm radio line using radio telescope RATAN-600. ... The existance of the large HI shell and a cavity in molecular gas distribution around Cygnus X indicates this radio source most probably to represent a united structure and whole gas may be drived by stellar wind of Cyg OB2 stellar assotiation. ...

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• Results scientific researchs LRS
• GRB follow-up team
• Results scientific researchs 24

The above image is a computer simulation of the distribution of mass in a Dark Matter dominated Universe. ... Structure (\eg density enhancements) clearly forms at the intersection of these filaments. ... What is Dark Matter? ... Testing for the presence of dark matter in the solar neighborhood now becomes an accounting problem The possible sources of this mass in the solar neighborhood are 1) luminous stars, 2) interstellar gas, 3) stellar remnants (mostly white dwarfs) and 4) dark matter: . ...

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Most current theories for magnetospheric emission can be grouped into polar cap, outer gap, and nebular models. These models, at least in some cases, need not be mutually exclusive; the Crab pulsar (among others), for example, shows clear evidence for pulsed emission from the magnetosphere and unpulsed emission from the surrounding nebula. ... This suggestion is strengthened by observation of a distinct soft emission component, consistent with the cooling scenario, from several of these pulsars. ...

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• Watching the Stars go `Round and `Round
• Conclusions
• *qpspec* - Extraction of Photon Distributions from QPOE files

... OCR by H.Andernach 1/96, to be proof-read) This is the first of a series of papers presenting results of a 10-GHz radio continuum survey of the galactic plane region using the 45-m telescope at Nobeyama. ... Weak Nonthermal Sources: A comparison with the Bonn S-GHz survey reveals a number of weak nonthermal sources near the galactic plane. ... For this reason we conducted a survey of the galactic plane region at 10 GHz using the 45-m radio telescope at the Nobeyama Radio Observatory (NRO). ...

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• Results and Discussion
• A CS and NH3 Survey
• Results of follow-up spectroscopy

T his page contains synthetic Hertzsprung-Russell Diagrams (HRDs) for a simulated Star Forming Region, assuming different scenarios and timescales for the history of star formation. ... In the paper we only presented the best fits to the HRD of the CMa R1 Star Forming Region. ... Download movie (1.90 MB) . Scenario II: Constant rate of star formation during a time interval delta t . delta t = 0.1 Myr . ... Scenario IV: Linearly decreasing rate of star formation during a time interval delta t . ...

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• AdelePlunkettAstro
• ESO - Thesis Topic: Discovery and characterisation of Pre Main Sequence stars
• Infrared/visible crossfade of the Monoceros R2 star-forming region | ESO

... We present the first results of an extensive near infrared survey of galactic and OH masers in high--luminosity star forming regions (SFR) aimed to see if there are near--infrared (NIR) sources directly associated with the masers. ... Although not in all sources there are high sensitivity--high resolution radio continuum observations, only few of the K--band/maser sources are closely associated with known ultracompact (UC) Hii regions. ...

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• Ronbun (Abstract)
• The BD+40 region (Abstract)
• Young stellar clusters in the star forming region NGC 6357

New 12CO J = 4-3 and 13CO J = 3-2 observations of the N 159 region, an active site of massive star formation in the Large Magellanic Cloud, have been made with the NANTEN2 and ASTE submillimeter telescopes, respectively. ... The 13CO J = 3-2 data were newly taken for the present work. ... The N 159 E clump is associated with cluster(s) embedded, as observed at 24н?m by the Spitzer MIPS, and the derived high temperature, 80 K, is interpreted as being heated by these sources. ...

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• HST this week: 267
• STScI Preprint #1276
• M3: An Ideal Laboratory for Testing Stellar Evolution and Dynamics

SWIRL DISTRIBUTION ON THE LUNAR SURFACE: LOCATIONS ANTIPODAL TO THE YOUNG BASINS? ... There are two main classes of hypothesises of the swirl origin: formation of the swirls in the regions antipodal to large impact basins (1), and formation of the swirls in result of cometary impacts (2). ... The Orientale basin is youngest. ... Fig. ... On the other hand, there are two cases of absence of correlation between swirl areas and regions antipodal to impact basins (for small swirl formations). ...

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• http://selena.sai.msu.ru/Symposium/ant.doc
• http://selena.sai.msu.ru/Shev/Publications/m44_76_sinitsin_shevchenko.pdf
• http://selena.sai.msu.ru/Pug/Publications/Pugacheva%20LPS%2041.pdf

Arecibo Galaxy Environment Survey (AGES) The M74 group is a gas-rich galaxy group located at roughly 10 Mpc and is similar in makeup to the Local Group. M74 dominates the surrounding region and is accompanied by several dwarf galaxies, some of which are star-forming. ... We have decided upon a drift mapping approach to scan the entire region. We have defined 5 constant declination scans 5 in length, separated by approximately one full ALFA footprint. ... START TIME (AST) . END TIME (AST) . ...

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• Colloquium Schedule
• The Arecibo Zone of Avoidance Survey (ALFAZOA)

... As is known, the observed distribution of massive stars in the direction of the Galactic center looks very peculiar: the vast majority of all massive stars are concentrated towards the central 1 pc or so (Genzel et al. ... In order to compare the observed distribution of X-ray sources in the Galactic center with what would be expected from the population synthesis computations, we have considered two hypothetical scenarios for the location of the starburst. ...

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• Parameters of the starburst
• Discussion and conclusions
• ADS Abstract Service Results

... We report on our ongoing project ``Infrared Study of HII Regions Associated with Small Clouds.' ... These IR data, combined with optical imaging (which will be obtained from the IAC-80 telescope), IRAS survey maps, and existing CO observations of the associated clouds, will allow us to undertake a detailed investigation of the gas-to-dust mass ratio, initial mass function and the star-formation efficiency in these complexes. ... CHECKPSF: check the PSF (Point Spread Function) model, . ...

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• Spatial Structure of NGC 6822: An Example for Statistical Modeling of
• INES Version 3.0: Functionalities and Contents
• On the Fly Bad Pixel Detection for the Chandra X-ray Observatory's Aspect...

T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...

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• David Nicholls: CV and publications
• Gemini Near-Infrared Integral-Field Spectrograph (NIFS) Science.
• The Milky Way in the region of the Southern Cross (Crux) and Centaurus rising

... Credit: ISAAC , 8.2-meter VLT , ESO Explanation: Star cluster RCW38 was hiding. This open cluster of stars is located about 5000 light years away towards the constellation of Vela . ... The reason is that the open cluster is so young that it is still shrouded in thick dust that absorbs visible light. ... When viewed in infrared light , however, the star cluster in RCW38 is revealed, because dust is less effective at absorbing infrared light. ... A Galactic Star Forming Region in Infrared . ...

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• Астронет > Star Forming Region RCW38
• Star Forming Region NGC 6357
• Star-Forming Region RCW38 from 2MASS

A water maser search towards colourґselected IRAS point sources By C l a ud i o C o d e l l ay AND F r a n c e s c o Pa l l az eґmail: codella@arcetri.astro.it y Dipartimento di Astronomia e Scienza dello Spazio, Universit`a degli Studi di Firenze, Largo E. Fermi 5, I--50125, Firenze, ITALY z Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I--50125, Firenze, ITALY The nature of 160 IRAS sources has been investigated through a search for water maser emission at 22.2 GHz. ... 100 Jy. ...

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• CO in NGC 1530, aperture synthesis of a barred spiral
• Sub-mm and radio observations of water maser sources
• Scaling relations for molecular gas in the Large Magellanic Cloud

... December 7, 1998 . Star-Forming Region RCW38 . ... Explanation: Star cluster RCW38 was hiding. This open cluster of stars is located about 5000 light years away towards the constellation of Vela . ... The reason is that the open cluster is so young that it is still shrouded in thick dust that absorbs visible light. ... When viewed in infrared light , however, the star cluster in RCW38 is revealed, because dust is less effective at absorbing infrared light. ... About APOD > . ...

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• APOD: 2006 December 20 - Star Forming Region NGC 6357
• APOD: 2008 March 12 - Star Forming Region LH 95
• APOD: 2004 November 1 - Spooky Star Forming Region DR 6

... Space Research Institute . Main . ... Main results of the experimental and theoretical research completed in 2010 . ... Moon's topography is shown based on LOLA laser altimeter data, white contour shows a permanently shadowed region and a white rhomb indicates LCROSS spacecraft impact location. ... Ultra deep survey of the sky in hard X-rays, performed by INTEGRAL observatory . INTEGRAL observatory has completed the first and the most sensitive survey of the sky in hard X-ray energy band. ...

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• The magnetosphere models
• Main results of the experimental and theoretical research completed in 2009
• SKA-3 Results Page

... High spectral, spatial and temporal resolution UV observations of the quiet Sun transition region show a highly structured and dynamical environment where transient supersonic flows are commonly observed. ... Estimates of the kinetic and enthalpy fluxes associated with these events show that explosive events are not important so far as solar coronal heating is concerned. ... In some cases, non-Gaussian line profiles are associated with supersonic flows in small magnetic loops. ...

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• Armagh Observatory
• Low-Mass Star Formation
• Observations and Data Reduction

... Star Atlas . ... stars . ... ALMA disentangles complex birth of giant stars . Observation results show the presence of multiple gas outflows from a protostar, indicating the possible existence of two newborn stars in the region. ... ALMA . ... It is the first time that such an hourglass structure was found in observations of methanol in high-mass star-forming regions. ... Observations with ALMA . ... It is thought that these gas clouds are surrounding a newly forming high-mass star like a cocoon. ...

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• Airborne observatory views star-forming region W40 | Astronomy.com
• As stars form, magnetic fields influence regions big and small | Astronomy.com
• ALMA probes environment around dark gamma-ray bursts | Astronomy.com