... Астронет | ... Star Forming Region S106 . ... Credit Copyright: GRANTECAN and IAC Explanation: Massive star IRS 4 is beginning to spread its wings. ... A large disk of dust and gas orbiting Infrared Source 4 (IRS 4), visible in dark red near the image center, gives the nebula an hourglass or butterfly shape. S106 gas near IRS 4 acts as an emission nebula as it emits light after being ionized , while dust far from IRS 4 reflects light from the central star and so acts as a reflection nebula. ...

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• Астронет > Mountains of Creation
• Астронет > Star Forming Region LH 95
• Астронет > M16: Pillars of Creation

... 2008 September 16 . W5: Pillars of Star Creation . ... JPL-Caltech , NASA . ... A likely reason for this is that the older stars in the center are actually triggering the formation of the younger edge stars. The triggered star formation occurs when hot outflowing gas compresses cooler gas into knots dense enough to gravitationally contract into stars. ... W5 is also known as IC 1848 , and together with IC 1805 form a complex region of star formation popularly dubbed the Heart and Soul Nebulas. ...

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• APOD: 2004 November 1 - Spooky Star Forming Region DR 6
• APOD: 2004 April 14 - Massive Star Forming Region DR21 in Infrared
• APOD: 2013 June 11 - Star Forming Region NGC 3582

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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• Read configuration information, create tables, and load data
• Infrared/visible crossfade of the Monoceros R2 star-forming region | ESO
• DFOS Installation: create ABs

... 2010, A , in press . SiO outflows in high-mass star forming regions: A potential chemical clock? A. Lopez-Sepulcre, C.M. Walmsley, R. Cesaroni, C. Codella, F. Schuller, L. Bronfman, S.J. Carey, K. M. Menten, S. Molinari, A. Noriega-Crespo . ... A comparative study of high-mass cluster forming clumps . ... Class I and Class II methanol masers in high-mass star forming regions . ... Click to examine publications from other years . ... Star Formation Group . ... Arcetri Home Page . ...

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• Create a www.arcetri.astro.it Mailing List

... SSAU History . SSAU roadmap . ... Scientists of SSAU and specialists of JSC Metallist-Samara work out a project on creation of import-substituting sea water desalting plants and wastewater treatment plants. ... So, the first experimental installation designed to produce one cubic meter of fresh water per hour, has a power consumption of only 10 kilowatt-hours, which is at the level of the latest foreign desalination plants. ... e-mail: ssau@ssau.ru . http://www.ssau.ru . ...

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• A chocolate printer is being created in SSAU
• SSAU and Swiss Centre CSEM will be engaged in the creation of electronic
• SSAU scientists are involved in the creation of a special 3D-printer for the

Next: Binary Radiopulsars with Black Up: Black Holes in Binaries Previous: Black Holes in Binaries . Two different types of stellar BH formation exist: (1) direct core collapse   of a massive star and (2) AIC of a NS. A BH of the first type presumably will have a mass comparable to that of the collapsing star and can be born both from a single star and in a binary system. ... Next: Binary Radiopulsars with Black Up: Black Holes in Binaries Previous: Black Holes in Binaries Mike E. Prokhorov . ...

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... Table files like the ones created in the section on imcnts can be displayed, printed and manipulated using the tasks contained in the stsdas.ttools package. ... sp> tables # Load the relevant package ta> tprint rp90_cnt prpar=yes # .tab extension assumed # the hidden parameter prpar is set to display the header # as well as the data ta> tprint rp90_cnt # Displays only the data info ta> tprint rp90_cnt prdata- prpar+ # Displays only the header info ta> tprint rp90_cnt prparam=yes | ...

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• Region Names and Colors
• Region Algebra
• The Markers Menu

... Our Galaxy . ... Stars . ... Space Flight . ... NGC 2841: a spiral galaxy some 46 million light years away. ... It is especially hard to explain this process of star birth in some spiral galaxies. ... Targets include both star clusters and galaxies, and star formation rates seen range from the starburst galaxy M82 (the Cigar Galaxy) which is creating about ten new stars in its core alone every year to the much less fecund star producer NGC 2841. ... Tweets that mention Baby stars of NGC 2841 | ...

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• The Solar System's Grand Tack | Astronotes

... If requested ( runbackground =Y), the task creates a background lightcurve, as well as a background spectrum for the imaging modes (FF, eFF, LW, SW) using background masks. ... The background masks are created by task badpixfind using threshold parameters, appropriate for the detection of real X-ray sources. ... As the GTIs strongly depend on the intended science this screening is not performed and only background masks, the lightcurve, and a GTI file are created by epchain . ...

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• Algorithm

... This is combined emission from all the gas clouds circling the black hole, between 0.1 and 10 light years out. ... These are the expanding clouds of gas left behind when a massive star comes to the end of its life and explodes, producing a supernova. ... Also known as the Veil nebula, a vast and beautiful whispy nebula left over from an exploding star. ... The Crab Nebula (120kb). ... Carbon Star (120kb) Red giant stars, surrounded by clouds or carbon dust. ... 3500 K star (64kb) , like Aldebaran. ...

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• Home Page of Raquel Salmeron

... To move toward open analysis software, we plan to make the PROS regions subsystem available from processes outside of IRAF. We also plan to make the region descriptor parsing system available for purposes beyond the creation of masks, such as an interface to an image display program, accepting a region descriptor and generating commands to display the region on an image. ... Anticipating two kinds of new requirements, we reconsidered the design of the PROS region descriptor processing subsystem. ...

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• ADASS 2002 Conference Proceedings
• Recreating Einstein Level One Processing Exposure Masks and Background Maps in
• A Method for Minimizing Background Offset Errors When Creating Mosaics

... The forcing by the solar wind is able to modify this field, creating a cavity called the magnetosphere. ... The outer boundary of the magnetosphere is called the magnetopause . In front of the dayside magnetopause another boundary called the bow shock is formed because the solar wind is supersonic. ... Solar wind and the magnetic field it carries along ( IMF ) modify the form of the magnetosphere, by pushing it in in the dayside and creating a long magnetotail in the nightside. ...

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• Ionosphere [Oulu]
• Heliosphere [Oulu]
• The Acceleration of the Aurora