A press release on the Canadian Galactic Plane Survey was associated with this poster. ... Below are maps of HI emission, HISA, and 12 CO emission in the eastern 25% of the survey, given as projections along the velocity ( Figure 1 ) and latitude ( Figure 2 ) axes. ... 2000, A. J. , submitted . ... GIF | ... We are developing automated methods of locating HISA in velocity cubes by removing large-scale emission in space and velocity and flagging small-scale dark residuals. ...

When: Tuesdays at lunch time (12:30 - 13:30). ... Tue, Aug 11: .. ... 070306: "Low Surface Brightness Galaxies" by Ralf-Juergen Dettmar . 140306: "Galactic Chimneys" by Naomi McClure-Griffiths . ... 090506: "Active Galaxies at high redshift" by Ilana Klamer . ... 050606: "Molecular Loops in the Galactic Center: Evidence for magnetic floatation to accelerate molecular gas" by Prof. Fukui . 130606: "Kinematical Studies of Ionized Gas in Nearby Dwarf Galaxies" by Janine van Eymeren . ...

... Dr. Stella Kafka . Thursday, Dec 10, 2015 at 8:00 PM . Type I Supernovae are massive stellar explosions that result from an interaction between a white dwarf and a companion whose mass it accrues in a close binary system. When the white dwarf’s mass reaches 1.4 that of the sun, the supernova occurs. ... Please join us for a pre-meeting dinner discussion at Changsho, 1712 Mass Ave, Cambridge, MA at 6:00pm before the meeting. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

Supermassive Black Hole Research: Session Overview . ... 2000. ... While black holes have long been hypothesized as the engines that power active galactic nuclei, conclusive detections and mass measurements long remained elusive. ... I will provide a brief overview of supermassive black hole research in general, aimed at providing listeners outside the subject area the context necessary for a proper understanding of the subsequent talks in the session. ... Last modified June 14, 2000. ...

... APT Activities and Science Results 3. ... APT Secretary Philip Edwards (ISAS) reviewed the aims of the APT (http://www.vsop.isas.ac.jp/apt/DefinitionAndAims.html). ... The Australia Telescope Compact Array, and Ceduna, Hartebeesthoek, Kashima, Mopra, Parkes, and Shanghai telescopes of the Asia-Pacific Telescope participated in these observations. ... In the absence of Tetsuo Sasao, Philip Edwards briefly described results of the APT 22 GHz observations conducted from October 1st to 5th, 1997. ...

... Science . ... The goal is to bring together two communitities: the one working on star formation (mostly galactic) and the one working on the formation of young massive clusters (mostly extra-galactic). We will link galactic with extra-galactic work, optical/NIR techniques with sub-mm/mm/radio ones, the formation of stars with the one of massive star clusters - observations and theory. ... Coordinated by Marina Rejkuba (abstract) . ... How did star formation proceed in Globular Clusters? ...

OptInt PmWiki : MROI Fast Tip Tilt / Tech Meet 4 . ... Attendees: JSY, MF, ADR, CAH, DFB, EBS, XS, DMAW . ... ADR & CAH: Layout and tolerancing of transmissive optical system . ADR & CAH: Use tolerancing results to assign image quality and stability budgets by component . ... MF: Thermal analysis of camera in box . ... Image Quality and Stability Criteria - Transmissive Systems (ADR) . ... Printable View of http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROIFastTipTilt/TechMeet4) ...

... Data . AAS 221 . AAS 219 . ... The first thing to note is that Twitter does not guarantee to return all matching Tweets, whatever method is used (unless you have direct access to their "fire hose", which I don't). ... This should result in the same results as my REST-based search (method 2), since the volume of Tweets was probably not enough to cause this site to miss Tweets based on their collection strategy . ... A search for the tag #aas219 (case insensitive) using the Twitter REST API . ...

Properties of the interstellar gas clouds . ... The angular resolution of this Survey was 2.4' x 130', velocity resolution was 6.3 km/s, r.m.s. fluctuations of antenna temperature (T a ) was 0.25 K. All clouds with kinematical distances r a Some selection effects were discovered and our statistic results were corrected for them. Figure 1. ... In the very high mass range the number of neutral gas clouds may be decreased because of gravitational instability or/and molecularization. ...

Armagh Observatory, 3 September 2001 . The Astronomical Science Group of Ireland ( ASGI ) meets in Armagh on Friday 7 September, for its autumn meeting to discuss new astronomical results obtained by Irish astronomers working both in Northern Ireland and the Republic of Ireland. The ASGI was formed in 1974 to provide a forum for the Irish astronomical community to meet on a regular basis and to exchange results and new information. ... Programme of Meeting . ...

Next: Other parameters of the Up: The Model Previous: Initial binary parameters . As we only deal with initially massive binary systems (their primary's mass is higher than 10 ), which are capable of evolving off the main sequence during less than years, the compact stars left behind stellar evolution are (in the case of the most massive stars) NSs and BHs. ... For a NS belonging to a binary, the evolution complicates as the secondary star evolves: for example, (recycling), etc. ...

... Meetings . ... List of all meetings from first one and up to present. Agenda of the session: eng version . ... Agenda of the meeting: eng version . Summary of the meeting: eng version . ... List of RISC members . ... List of participants . ... Agenda of the meeting: eng / rus version . ... Formal minutes: eng version . ... Lists of participants: eng / rus version . Formal minutes: eng / rus version . ... Agenda of the meeting & List of participants . ... Agenda of RISC's meeting . ...

ESAC Trainee (Alumni) Meeting, 24-Jul-2006, ESAC . ... XMM-Newton SOC Home Page Conferences & Meetings . ... SOC Info XMM-Newton Contact Details How to get to ESAC ESA Research Fellowships ESAC Trainee Projects ESA Young Graduate Trainees . ... Trainees from various Universities and the ESA Young Graduate Trainee Programme are involved. The trainees as of now have been from the following universities: . University Complutense de Madrid (Spain) . University of Bonn (Germany) . ... ESAC . ...

Next: A candidate young galaxy? Up: Results and discussion Previous: Current star formation rate . The integrated H I line flux, the characteristic widths of 21 cm line profile W 50 and W 20 (for a Hanning smoothing of 10.6 km s -1 ), and the derived H I mass for HS 0822+3542 are presented in Table 1 . The small H I mass 2.4 of this galaxy is consistent with its low optical luminosity. ... A rough estimation can be made also on the dynamical mass of HS 0822+3542. ...

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... Mass . 17a. Measuring Mass . ... A medium-size (1.25 inch wide) binder clip, as is used in offices to hold papers together--the type made of flat blue steel, with two wire handles. ... The theory predicts that the oscillation period should be proportional to the square root of the oscillating mass, including the mass of the clip. Note that gravity plays no part here: the oscillation period would be the same on the Moon or in zero-g. Denoting square root by SQRT, we have . ...

3) Planets and Brown Dwarfs . ... By its nature, this method is most sensitive to massive planets orbiting close to their stars. ... That means that some of the more massive extrasolar planets could actually be brown dwarfs (although the statistics of the finds suggest that most of them are not). ... Another possible difference between brown dwarfs and massive planets is how they are born. ... They would base the fundamental definition on the mode of formation: a planet is built from planetesimals. ...

BaBar Collaboration Meeting , December 6-10, 2004 . ... APS April Meeting 2004 , May 1-4, 2004 . ... Workshops in Particle Physics , February 29 - March 6, 2004 . ... Aspen 2004 Winter Conference on Particle Physics , February 1-7, 2004 . ... Exp Talks - Prior Years . ... Energy Spectrometer Designs and Beam Tests , Eric Torrence . ... Recent Results from the LIGO Experiment, Isabel Leonor . ... Experimental Introduction , Ray Frey . ... CCD R at Oregon University , Nick Sinev, Olya Igonkina . ...

... ROTATION CURVE: When studying spiral galaxies it is invariably found that the stellar rotational velocity in the disk remains constant, or "flat", with increasing distance away from the galactic center. ... The rotation speed of the stars in galaxies is found NOT to decrease with increasing distance from the galactic center (see emission lines in the spectrum), implying that the overall mass distribution of the galaxy is different from the light distribution. ...

... Credit: W. Pounds Explanation: It's clear who is the biggest star in this binary system. Based on recent results , this artist's vision of the double star Phi Persei , 720 light years away, shows a bright, rapidly rotating massive star surrounded by a disk of gas. A small companion star orbits 100 million miles away. ... Astronomers consider the ultimate fate of such mass-exchanging, interacting binary systems an open question and a challenge for present theories of stellar evolution . ...