Observed maximum rotation velocity uncorrected for inclination effect. This quantity is calculated from 21-cm line widths at different levels and/or rotation curves (generally in H_alpha). ... These data are characterized by some secondary parameters: telescope, velocity resolution, level of the 21-cm line width and bibliographic reference. ... we start from a standard sample (a set of measurements giving a large and homogeneous sample). ... HyperLeda . ...

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• HyperLEDA: compilation of central velocity dispersion
• HyperLEDA documentation: parameter: vmaxs
• HyperLEDA documentation: catalogue of internal kinematics

... We have mapped the 21-cm absorption in the nuclear region of the starburst galaxy NGC 1808 using the VLA AnB-hybrid array with a resolution of approx. 5.2" (= 275 pc). ... The velocity center of the absorption changes from about +120 km/s relative to the systemic velocity in the NW to -145 km/s in the SE, following the rotation pattern in the outer regions of the galaxy. ... The gravitational mass required to explain this fast rotation in the center of NGC 1808 is a few times 10^9 solar masses. ...

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• ROTATION-CURVES tasks
• Fitting a rotation curve
• The Structure of Dark Halos: Model-Independent Information from HI Rotation

... MADS] data depth? Tags: break points , data depth , MADS , mean , median , multivariate , nonparametric , order , parasite , quantile , robust , sort , vertebrate . ... Tags: biased , breakdown point , chi-square , confidence interval , coverage , delta chi-square , estimator , LAD , mean , median , plug-in , rmse . ... The breakdown point of the mean is asymptotically zero whereas the breakdown point of the median is 1/2. ... Tags: breakdown point , mean , median , quantile . ...

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• Rotation Periods of ZAMS Stars
• The AstroStat Slog mean
• Direct Monitoring of Rotational Modulation

... Makarov D.I., Karachentsev I.D., Burennkov A.N., Tyurina N.V., Korotkova G.G. "Rotation curves of edge-on galaxies" . ... Karachentsev I.D., Makarov D.I., Sharina M.E., Dolphin A.E., Grebel E.K., Geisler D., Guhathakurta P., Hodge P.W., Karachentseva V.E., Sarajedini A., Seitzer P. "Local galaxy flows within 5 Mpc" . ... Karachentsev I.D., Makarov D.I. "Local Field of Galaxy Velocities" . ... Karachentsev I.D., Makarov D.I. "The Galaxy Motion Relative to Nearby Galaxies and the Local Velocity Field"...

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• INASAN preprint: A method of the reconstruction of 3D velocity field of gas in
• Results scientific researchs LRS
• Laboratory of spectroscopy and photometry of extragalactic objects : Vortex

... According to the most popular cosmological paradigm, the greater part of the galaxy mass is accumulated in the dark matter halo. ... The polar ring galaxies (PRGs) reveal external rings or disks of gas, dust and stars rotating in a plane roughly perpendicular to the disk of the central galaxy. ... The shape of the dark halo in the model was chosen so as to achieve the best fit to the observed rotation of both galaxies themselves and their polar rings. ... The SPRC-7 galaxy. ...

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... The first column shows the kinematical diagrams, where is the angle between the line of sight on the object and the vector of rotation about Z -axis, and V S is objects line-of-sight velocity relative to an observer at rest at the position of the Sun. The straight lines are regression fits, whose slopes yield the subsystem’s rotation rate. The second column shows the relations between metallicity and distance from the Galactic plane. ... privious figure | next figure . ...

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• Vladimir Marsakov Abstracts
• Vladimir Marsakov Publication List

Globular Clusters as Dynamical Probes of the Virgo Giant Elliptical M49 T.J. Bridges et al. Anglo-Australian Observatory, Australia We have obtained spectra and velocities for 144 globular clusters in the Virgo giant elliptical M49, and are using these data to study the kinematics, ages and abundances of the globular clusters, and the dynamics, dark matter content, and origin of M49. ... We con rm X-ray evidence for a dark matter halo in M49, nding a M/LB  70 at 50 kpc galactocentric radius. ...

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... Subject and Problems of Stellar Astronomy. ... Plane of Galaxy, Methods of Its Location Determination. ... Stars Distances. ... Other Methods of Stars Distances Determination. ... Tangential Velocities, Their Determination by Self-Motions. ... Determination of Solar Apex and Spatial Velocity by Radial and Spatial Velocities of Stars. ... Features of Orientation and Parameters of Peculiar Stellar Velocities Ellipsoid. ... General and Selective Light Absorption in Galaxy. ... Darc Clouds in Galaxy. ...

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• Introduction to Astronomy
• Spherical and Practical Astronomy

... Same Visit, No Rotation, Large Shift . ... Data . ... HST Overview . Overview . ... Retrieving HST Data . ... Data Analysis . ... This IDCTAB contains uniquely computed distortion solutions for 10 filters: F225W, F275W, F336W, F390W, F43W, F555W, F606W, F775W, F814W, and F850LP. All other filters use the values for F606W. This test is designed to determine how the IDCTAB deals with a large shifts. ... F606W . ... X RMS Y RMS Vec Mag RMS Vec Mag Mean Vec Mag Median Vec Mag Max Vec Mag Min . ...

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• No Shift, 180 Degree Rotation
• Same Visit, No Rotation, No Shift
• Nuclear, Stellar Disks in E/S0 Galaxies

... NGC1850: Star Cluster in the LMC . ... NGC1850 is a large cluster of stars located a mere 166,000 light-years from Earth in our neighboring galaxy the Large Magellanic Cloud (LMC). ... Arp 220: Spirals in Collision . ... Arp 220 is the brightest object in the local universe. ... Arp 220 was cataloged as a peculiar galaxy in the 1960s. In the late 1980s, it was discovered to be an ultraluminous infrared galaxy and headed a list compiled from observations with the now-defunct IRAS satellite. ...

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... 24sep08: long recovery vs alfa rotation angle. ... On 23sep08 around 14:00 hours data was taken with alfa on the sky to see how long the recovery took. ... 2 172 MHz Bands per beam . ... On 24sep08 around 17:00 data was taken with alfa and the pdev spectrometer to measure the long recovery time versus the rotation angle of alfa. ... As alfa rotates, different beams have larger/smaller recovery times. ... This is the same data as the total power plots above. beam 0 alfa rotation= 0 deg . ... page up ...

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• rotary floor
• Slide 2
• rotaPlatToSky

... l - the mean galactic longitude; . ... mul - the median proper motion along galactic longitude of the stars of the OB-association, in units of 0.001 arcsec year -1 ; . dml - the estimation of mul dispersion in the OB-association, in 0.001 arcsec year -1 ; . mub - the median proper motion along galactic latitude of the stars of the OB-association, in units of 0.001 arcsec year -1 ; . dmb - the estimation of mub dispersion in the OB-association, in 0.001 arcsec year -1 ; . ...

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... We present high angular resolution millimeter wavelength continuum and 13CO(2-1) observations of the circumstellar disk surrounding the TTauri star DG Tauri. We show that the velocity pattern in the inner regions of the disk is consistent with Keplerian rotation about a central 0.67 Msun star. The disk rotation is also consistent with the toroidal velocity pattern in the initial channel of the optical jet, as inferred from HST spectra of the first de-projected 100 AU from the source. ...

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• rotatelogs - Piped logging program to rotate Apache logs - Apache HTTP Server
• Accomodation - Cosmic Polarization Rotation Workshop, September 7-8, 2015
• Programme - Cosmic Polarization Rotation Workshop, Septemeber 7-8, 2015

... Lesson plan (frames) . ... 22b. Relativity . ... By Newton's laws, two frames of reference moving with constant velocity relative to each other observe exactly the same physical behavior. There exists no way to tell, which of them is moving and which one is at rest: there is no "absolute rest frame" and no "absolute (constant) velocity. ... But for a while it seemed that by certain subtle effects, electromagnetic forces could distinguish whether a frame was in motion of not. ...

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• Frames of Reference: The Basics
• Flight to Mars: the Return Trip
• The Rotating Earth

... Bad Astronomy . Misconceptions . ... Bad Astronomy : The Moon only shows one face to us because it is not rotating. Better astronomy : The Moon only shows one face because it is rotating, once every time it revolves around the Earth. ... Place the Moon model on the table about 30 centimeters (one foot) away with the X facing the Earth model. ... You'll see that to keep the X facing the Earth model, you have to rotate the Moon model as it goes around the Earth model . ... 2008 Phil Plait. ...

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• Phil Plait's Bad Astronomy: Bad News

... To derive the motion of a penny dropped inside an airliner moving at 600 miles/hr (about 1000 km/hr)--should we calculate it with respect to the interior of the airliner, or with respect to the ground? ... And if a similar penny is let go inside an orbiting spaceship--should its motion be calculated relative to the interior of the spaceship, or relative to the Earth outside? ... Each such choice is known as a frame of reference . Some possible frames are -- the interior of the airliner, . ...

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• Motion in a Circle
• Frames of Reference: The Centrifugal force
• Concerning Steady State Corotation of the Io Plasma Torus

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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• Dark Matter in Spiral Galaxies
• Mars rotating
• Lecture 15: Rotation and Angles

... 2010 January 24 . Watch Jupiter Rotate . Credit: NASA , Johns Hopkins University Applied Physics Laboratory , Southwest Research Institute . Explanation: What would it be like to coast by Jupiter and watch it rotate? This was just the experience of the New Horizons spacecraft as it approached and flew by Jupiter in 2007. ... Other movies compiled by New Horizons and other passing spacecraft have captured the clouds swirling and moving relative to themselves. ... About APOD | ...

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• APOD: 2011 June 1 - Earth Rotating Under Very Large Telescopes
• APOD: 2014 March 12 - The Sun Rotating
• APOD: 2000 October 24 - Io Rotating

... I built a Master Catalogue of stars towards the Magellanic Clouds (MC2) based on multiwavelength cross-identifications of the DENIS , 2MASS , GSC-II and UCAC point source catalogues. ... See http://vizier.u-strasbg.fr/MC2/ . ... Nous avons rИalisИ un "Master Catalogue of stars towards the Magellanic Clouds" (MC2) basИ sur l'identification croisИe multi-longueur d'onde des catalogues de sources ponctuelles DENIS , 2MASS , GSC-II et UCAC . ... Voir http://vizier.u-strasbg.fr/MC2/ . ...

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• Rotating stars
• ESO - Thesis Topic: Optical interferometric imaging of rapidly rotating stars
• Rotation of the disc in M 17 | ESO

... 8, ``Celestial Mechanics'', 2002 Generalized Nordtvedt effect and tests of equivalence principle for rotating bodies Yu. ... To study theoretical predictions for possible violation of EEP the Thirring­Feynman field gravity theory (FGT) is considered [3], [4]. ... Using Lagrangian formalism of the relativistic field theory the post­Newtonian equation of translational motion for rotating bodies is derived in the frame of FGT. ... Thirring W. Field--theoretical approach to gravitation. ...

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• LAB Space Geodesy and Earth Rotation - QUASAR
• LAB Space Geodesy and Earth Rotation-GRAPE
• LAB Space Geodesy and Earth Rotation-OCCAM/GROSS