... However, the comparison of masses deduced from the continuum SIMBA 1.2 mm emission and virial masses (understood to trace the entire potential of the clouds) in a sample of giant molecular clouds in the Small Magellanic Cloud (SMC) by previous studies found a discrepancy between these two quantities that requires explanation. ... Methods: New observations of the southwest region of the SMC were obtained with the LABOCA camera on the APEX telescope. ...

Еще в разделе: (Показать все результаты (>16677) - www.stsci.edu/ )

• The State of the Gas and the Relation between Gas and Star Formation at Low
• Far-Infrared Observations of Radio Quasars and FR II Radio Galaxies
• Dust/gas correlations from Herschel observations

All stars are formed deep inside molecular clouds. One of the current enigmas lies in the formation and evolution of molecular clouds, specifically the conversion from atomic to molecular gas. ... In July of 2005 GALFA mapped about 300 square degrees of the Taurus Molecular Cloud (TMC) complex yielding the largest high-resolution 21cm map of a star forming region, while using less than 40 hours of observing time. ...

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• Heiles Symposium Presentations

... Using the obtained above dependence of compact binary merging rates in the elliptical galaxy on time (Fig. ) and assuming the cosmological origin of GRB as products of binary NS/BH coalescences, we can compute the theoretical - curve. ... Figure: (Right panel) The 2-nd BATSE catalog (solid points) is fitted by the cosmological GRB model (from Lipunov et al. ... Note that the total GRB rate in the Universe is per year, 3 orders of magnitude smaller than the total binary NS merging rate. ...

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• Scientific Interests
• Vladimir Mikhaylovich Lipunov

... Radio emission at around 90 GHz from star-forming galaxies is expected to be strongly dominated by the free-free component due to ionising radiation from massive, short-lived, stars. We present high surface-brightness sensitivity observations at 90 GHz of the nearby star-forming galaxy Messier 66 with resolution of about 9 arcsec (corresponding to a physical scale of about 500 pc) and analyse these observations in combination with archival lower frequency radio and mid-infrared measurements. ...

Еще в разделе: (Показать все результаты (>2356) - www.mrao.cam.ac.uk/ )

• Publications | Matt Bothwell
• G111.7-2.1
• G184.6-5.8

Hot Molecular Cores at Mopra Molecular line observations of star-forming regions 2000­2002 Cormac Purcell, Ramesh Balasubramanyam, Lucyna KedzioraChudczer, Vincent Minier, Tracey Hill, Michael Burton, Maria Hunt, Peter Barnes, Jill Rathborne. Cormac Purcell, Star Formation Group, UNSW. ... High abundances of saturated hydrocarbons fuelled by evaporation from icy grainmantles · n(cm-3)~107 100K<T<300K 0.05pc<0.1pc Cormac Purcell, Star Formation Group, UNSW. What is a `Hot Molecular Core'? ...

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• Programme - Abstract
• Molecular gas
• The optical emission from gamma-ray quasars

... J. Brand, M. Felli, R. Cesaroni, C. Codella, G. Comoretto, S. Di Franco, F. Massi, L. Moscadelli, R. Nesti, L. Olmi, F. Palagi, F. Palla, D. Panella, R. Valdettaro . 2007, IAU Symposium 242, p. 223 . ... 2007, ApJ, in press . ... Murphy, G. C., Lery, T., O'Sullivan, S., Spicer, D., Bacciotti, F., Rosen, A. 2007, A , in press . ... Rubini, F., Lorusso, S., Del Zanna, L., Bacciotti, F. 2007, A , in press . ... Coffey, D., Bacciotti, F., Ray, T.P., Eisloeffel, J., Woitas, J. 2007, ApJ, in press . ...

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• Arcetri Star-formation Group Research Topics
• A local window on galaxy formation with ALMA
• The puzzling core of the Phoenix cluster: deep X-ray observations

... 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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• Plasma sheet high speed flows [Oulu]
• Brief History: Convection
• Upward flowing ions [Oulu]

... This CCF contains the following five extensions: ADUCOEFF , OFFSET_GAIN , GAIN-HIGH , REEMISSION and REEMISSION1 . ... Code of the bad pixel table (BPT) version, which includes the additional column offset values, described in the OFFSET_GAIN extension. ... GAIN : . ... Vector column of length 64; one gain value per node per chip. ... Vector column of length 64; one offset value per node per chip. ... Vector column of length 64; constant in linear offset value calculation (only present for ALGOID =1...

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• Selection of observations of empty RGS files
• XMM-Newton SAS: Watchout Page

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies using ALMA calibrator observations . ... ALMA . ... ESO-MIDAS . ... It is therefore essential to probe the evolution of cold gas over cosmic time. ... We are looking for an enthusiastic PhD student who is interested in working with us in using ALMACAL to address exciting and topical science questions related to the evolution of molecular gas in galaxies. ...

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• ESO - Star and Planet Formation Workshop
• Research
• ESO - ESO sky correction tools

... Huchtmeier Richter A catalog of all published HI observations of external galaxies has been compiled. ... the morphological type (internally coded in a crude 1-byte code based on the system of the RC2 Second Reference Catalog of Bright Galaxies (de Vaucouleurs et al, 1976)) in column 4; . the inclination i (in degrees) used by the authors in column 5. ... A General Catalog of HI Observations of External Galaxies by W.K. Huchtmeier O.-G. Richter, H.D. Bohnenstengel and M.Hauschildt May 1983. ...

Еще в разделе: (Показать все результаты (>2625) - www.sao.ru/ )

• Format conversion
• Blue Compact Galaxies from the Hambyrg/SAO Survey
• Reducing the observations

... I will discuss how observations of synchrotron intensity fluctuations can be used to probe the sonic and Alfvenic Mach numbers of interstellar turbulence, based on mock observations performed on simulations of magneto-hydrodynamic turbulence. I will also discuss the potential for novel polarisation analysis techniques to uniquely determine the sonic and Alfvenic Mach numbers of observed turbulence, and to assist in qualitative understanding of Galactic magneto-ionic turbulence. ...

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• http://www.mso.anu.edu.au/seminars/abstracts/20150206-1400.html
• http://www.mso.anu.edu.au/seminars/abstracts/20160407-1100.html
• ANU - Research School of Astronomy and Astrophysics - 5th Stromlo Symposium

11 august 2014/Monday: Arriving, Registration . ... The variation of solar flare coronal X-ray source spatial properties. ... Melnikov V.F., Charikov Yu.E., Kudriavtsev I.V. Directivity of X-ray and gamma-ray emission from different parts of flaring magnetic loops. ... E., Melnikov V.F. Angular characteristics of polarization degree of hard X-ray emission from different parts of flaring magnetic loops. ... The thick target model and analytical calculations of the hard X-ray emission from solar flares. ...

Еще в разделе: (Показать все результаты (>304) - www.gao.spb.ru/ )

• Pulkovo NEO Page: Observations

... Наблюдательные характеристики областей образования массивных звезд . ... Anglada G., Estalella R., Pastor J. A CS and NH 3 survey of regions with H 2 O maser emission // Astrophys. ... Rev. Astron. Astrophys. ... Bonnell I., Bate M.R., Zinnecker H. On the formation of massive stars // Mon. ... Astron. ... Cabrit S., Bertout C. CO line formation in bipolar flows. ... Зинченко И.И. Статистика высокоскоростных потоков в областях образования массивных звезд // Письма в АЖ, в печати . ...

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• Journal "Peremennye Zvezdy" > PZ: main journal.
• Journal "Peremennye Zvezdy"
• XWare > APOD

Next: Public Understanding of Science, Up: Technical Research Summaries Previous: New Approaches to Risk . ... Michael Smith has been analysing new infrared data collected from 11 PPN and PN by Chris Davis (Joint Astronomy Centre, Hawaii) to search for clues as to how the objects evolve. ... Georgi Pavlovski studied the properties of supersonic turbulence in molecular clouds and its effect on the molecular cloud properties and their chemical evolution. ...

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• Armagh Observatory
• Observations with the Faulkes Telescopes
• Jorick Vink

... GCN 1488 . ... GCN 2001 , 2024 , 2046 , 2051 , 2054 , 2079 , 2094 , 2105 , 2108 , 2119 , 2198 , 2204 , 2220 , 2260 , 2299 , AstL (2003) , ApJ (2004) . ... GCN 2821 , 2826 , ApJ (2010) . ... GCN 3139 , ApJ (2010) . ... GCN 3493 , ApJ (2010) . ... GCN 3718 , ApJ (2010) . ... GCN 3853 , 3864 , 3896 , ApJ (2010) . ... GCN 5173 , 5177 , 5183 , 5186 , 5189 , 5193 , AstL (2007a) , AstL (2007b) , A (2010) . ... GCN 5524 , ApJ (2010) . ... GCN 9037 , ApJ (2010) . ... Russian-Turkish 1.5-m Telescope (RTT150) ...

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• z90-program
• Fast search through RTT150 data archive
• The 6th INTEGRAL Workshop "The Obscured Universe"

Next: Emission molecular bands Up: Optical spectrum of IRAS04296 Previous: Optical spectrum of IRAS04296 . We have obtained spectra of IRAS04296 with the CCD (1140 1170 pixels) equipped echelle spectrometer PFES mounted at the prime focus of the 6m telescope of SAO RAS (Panchuk et al. ... Figure: The IRAS04296+3429 spectrum near . Next: Emission molecular bands Up: Optical spectrum of IRAS04296 Previous: Optical spectrum of IRAS04296 Klochkova V.G. 12/20/1999 ...

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• Emission molecular bands
• GRB follow-up team
• Optical spectrum of IRAS04296

2012 A Broadband Study of the Emission from the Composite Supernova Remnant MSH 11-62 (P. Slane et al.) ... 2012 Infrared imaging and polarimetric observations of the pulsar wind nebula in G21.5-0.9 (A. Zajczyk et al.) ... 2009 High-resolution X-ray Observations of the Pulsar Wind Nebula Associated with the Gamma-ray Source HESS J1640-465 (A. Lemiere, P. Slane, B.M. Gaensler, S.S. Murray) - ApJ, 706, 1269 . ... 1995 Soft X-Ray Emission From Selected Isolated Pulsars (P. Slane N. Lloyd) ApJ 452, L115 . ...

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• An Example - 3C 120
• Pat Slane: Pulsar Page
• Magnetospheric Emission From Isolated Pulsars

. IKI follow-up GRB team . Crimean Astrophysical Observatory . Special Astrophysical Observatory . Contact information | IKI main page .

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• CYlindrical GAmma-ray Monitor CYGAM -
• Events on January 10-11, 1997 - INTERBALL observations
• Brief History: Convection

... Aloisi, A. The Old Stellar Population . Alonso-Herrero, A. HST /NICMOS Observations of the . ... Balcells, M. HST-NICMOS Observations of Galactic . ... Baum, S.A. Investigating the Evolution of . ... Becklin, E.E. A Coronagraphic Search for . ... Clampin, M. The Old Stellar Population . ... Close, L. HST NICMOS Observations of . ... The Stellar Population in . Geballe, T.R. HST NICMOS Observations of . ... Greggio, L. The Old Stellar Population . ... Leitherer, C. The Old Stellar Population . ...

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• NICMOS Science
• Limits on the Star Formation Rates of z>2 Damped Ly Systems from H Spectroscopy
• HST/NICMOS Observations of the Interacting System Arp 299

... Field of interest: data analysis and interpretation of X-ray observations of BHC and NS systems, astrophysics of compact objects and related phenomena: X-ray , optical and radio observations , shocks and stellar winds, emission mechanism, the spectral and timing analysis of the X-ray emission from microquasars ( signature of accreting BH), atoll- and Z-sources ( signature of accreting NS), modeling of INTEGRAL images % . ...

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• Igor Antokhin