Scale-heights of the Galactic disk subsytems with different ages and metallicities . V.Marsakov & Yu. ... It is based on the fact, that all stars cross the disk plane several times during their Galactic orbital period. ... We have used our representative sample of nearby disk F2-G2 stars Marsakov & Shevelev (1995) in which fundamental stellar parameters was determined on the basis of published date on uvby-photometry, proper motion and radial velocities. ... Marsakov V.A., Shevelev Yu.G. Bull. ...

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• Vladimir Marsakov Abstracts
• F-stars in galactic disk, figures

Next: The Scenario Machine: Operational Up: Evolution of Magnetic Rotators Previous: Ejector-propeller hysteresis . ... The length of this segment is determined by the eccentricity. ... In this case no hysteresis occurs and transitions E -- P and the reverse take place in symmetrical points of the orbit. ... Here EP means a mixed state of the rotator at which it is in the ejector state during one part of the orbit, and in the propeller state during the rest of the orbital cycle. ...

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• Gravitational waves from supernova explosions

Next: Cosmological Molecular Clouds Up: HST and the Previous: Cepheids in NGC . ... Recent calibrations of stellar surface brightness derived by modern observational interferometry show that the Cepheid PLC relations turn out to be much less affected by abundance effects than PL ones. Extragalactic Cepheid distances revisited by a calibrated PLC (V, V-Ic) relation indicate some significant systematic shifts affecting current PL determinations achieved by ground-based and HST photometry. ...

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• Andy Fruchter's Homepage
• Gauging the impact of executing science program across different COS/FUV
• How are the reference data named, and how do i differentiate the different file

... Archives . ... If you do not mind the time predictor, it is hard to believe that this is a light curve, time dependent data. ... It?s hard to say this data set is designed for time series analysis apart from the complication in statistical inference due to measurement errors. How to design the statistical study with measurement errors, huge gaps in time, and unequal time intervals is complex and unexplored. ... The following is R output without measurement errors. ... Chandra Blog . ...

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• zhtools
• The Orion OB1 Association
• The AstroStat Slog outliers

... Colours of stars and galaxies hold information on intrinsic and extrinsic parameters, such as stellar temperatures and galaxy populations, selective absorption and colour changes due different dust contents and inclination angles of galaxies, as well as galaxy redshifts and evolution. ... The colour magnitude diagram of 65000 galaxies to which all above-mentioned quantities and others contribute can only be explained by comparison with simulations. ... Colours are also of technical help. ...

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• ESO - I want to process MOS data of the same target from different nights
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• Different X-ray Spectra

Fabry-Perot data cubes. Introduction: what is "data cubes"? Observations with the IFP consist of successive acquisition of a few dozen images of interference rings from the object (or from a calibration lamp) when changing the optical path between the flat-parallel plates. The radius of the rings is a function of wavelength and gap between the plates of the interferometer. ... Its interference rings of Ne line which use for phase calibration (convert object data to wavelength-scale). ...

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• Work Scan Program + Data Viewer (IDL widget)

Dense Gas in the LMC and the Circumstellar Shell of R Scl Tony Wong, ATNF Millimetre Workshop 21 Nov 2002 With: John Whiteoak, Maria Hunt, Michael Lindqvist, Hans Olofsson 1. ... 1997 · SEST 58" beam · Tmb(HCO+) 0.6 K · Flux 15 Jy Fukui et al. 2001 3 Massive Star Formation in N113 NANTEN CO contours over H image from Kennicutt 4 First ATCA Observations HCO + · 9 Jul 2001, single baseline · Additional observations on 10 Jul and with 3-element system on 4 and 8 Oct. ...

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• http://www.atnf.csiro.au/research/LVmeeting/magsys_pres/sydneyMC160707.pdf
• Input Parameters to the Self-Calibration Tasks
• Self-Calibrating with Multiple Models

... Slide 2 . ... Smooth Accretion of Intergalactic Gas . Mergers and Satellite Accretion . Galactic Fountain Material . HIPASS = HI Parkes All-Sky Survey . A typical HIPASS data cube . HIPASS was designed to be an extragalactic survey . ... Different types of HVCs in different environments? ... HVCs and Galactic Emission . ...

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• Different types of HVCs in different environments?
• new 12m antenna for Arecibo
• rotaPlatToSky

... Clearing the library. Note the different flooтАж . Sidebar Left . Sidebar Top . ... Title: Clearing the library. Note the different floor levels. There were at least 4 different levels of underfloor in the library. Description: NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ... NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ...

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• Wavelengths
• Things are very different for small planets
• Lesson 1: Plotting Data with Excel

... The greater the distance, the smaller the parallax. ... That triangle has the same proportions as the much larger triangle ABC, and therefore, if the distance B'C to the thumb is 10 times the distance A'B' between the eyes, the distance AC to the far landmark is also 10 times the distance AB. ... The most distant objects our eyes can see are the stars, and they are very far indeed: light which moves at 300,000 kilometers (186,000 miles) per second, would take years, often many years, to reach them. ...

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• Polar Orbiting Satellites
• Electromagnetic Waves
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... sin f = y / r . cos f = x / r . ... They are now viewed as new definitions of the sine and cosine, for the polar angle f given by x and y ( a slightly different way of formulating this definition is described further below ). ... sin 2 f + cos 2 f = 1 . ... Angle . ... Many trigonometry texts define the sine and cosine slightly differently, using the so-called unit circle . ... Then the distance AB ("the sine line") equals sin a , and the distance OA ("the cosine line") equals cos a . ...

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• Space Research Institute (IKI) Seminar
• Polar Orbiting Satellites
• INTERBALL Tail Probe flight longterm situation analysis 1995 - 2000

... In order to disentangle the effects of different climate variables on tree-ring growth rates of different species, and to explore the possibility that more than one species could improve the accuracy of the reconstructions of climate using tree rings, a methodical study of trees in close proximity to the Armagh Observatory climate station was initiated together with Ana Maria Garc?a Su?rez, and continued as part of the latter's PhD thesis with John Butler and Professor Mike Baillie (QUB). ...

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• Armagh Observatory
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• Armagh Astropark

... March 16, 1998 . Asteroids in the Distance . Credit: R. Evans K. Stapelfeldt ( JPL ), WFPC2 , HST , NASA . Explanation: Rocks from space hit Earth every day. The larger the rock, though, the less often Earth is struck. Many kilograms of space dust pitter to Earth daily. ... Many asteroids remain undiscovered. ... Such an interplanetary collision would not affect Earth's orbit so much as raise dust that would affect Earth's climate . ... About APOD > . ... NASA Technical Rep.: ...

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• APOD: 2013 February 10 - Asteroids in the Distance
• APOD: 2005 April 17 - Asteroids in the Distance
• APOD: 2007 November 19 - Aurora in the Distance

Auxiliary table the distance catalog . HyperLeda home | Documentation | Search by name | ... Search an object in the distance catalogue . The table auxdistance contains homogenization parameters for different datasets and methods. It implies a linear relation in the form Y=a*X+b. The default values are a=1 and b=0 which means NO any correction will be applied. ... It is a bibliographic reference in HyperLEDA database which reffers the bref04 table. ... REAL NOT NULL . ... REAL . ...

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• Getting the Dispersion Solution
• Results and discussion
• Correspondence Analysis

... A detector map is used to provide a grid of positions over which to calculate and flux weight the ARF. The default detector map is 'flat' which has a weighting of 1.0 for each detector map pixel and is rectangular having sides which just encompass the region specified in the DSS. Only detector map pixels falling within the source region are included in the ARF calculation, e.g. for a circular source box, the pixels in the corners of the detector map will be ignored. ... flat : . ...

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• Procedure
• Generation from Ground Calibration Data
• Description

.

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• Astronomy HyperText Book: Stellar Clusters
• Astronomy HyperText Book: Stellar Evolution
• First Steps to the Renaissance

. There are several different shells available for Unix; the most popular are described here. You can use any one of these shells if they are available on your system. And you can switch between the different shells once you have found out if they are available. Bourne shell (sh) . C shell (csh) . TC shell (tcsh) . Korn shell (ksh) . Bourne Again SHell (bash) .

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• Using a different printer
• Example of using a different printer
• Different types of file

The Mars Flag has a different design on the reverse side. obverse side of flag . ... The orbit lines on the obverse cross the Sun on the lower half of the flag and appear to go behind the Sun on the upper half of the flag. The reverse side has the orbits lines continuing around the Sun on the upper half of the flag. ... The Mars Flag reverse side is a continuation of the obverse side and not just a different design on the back and not a mirror image of the obverse. Main Flag Background Color . ...

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• ASP: Using Multicultural Dimensions to Teach Astronomy
• ASP: Steering by Different Stars? Astronomers and the Dark-Sky Movement
• ASP: A Taste of Real Astronomy ? The ESA/ESO Astronomy Exercises

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• Extinction properties (transmitted radiation)
• Database of Optical Properties -- Level: subpage
• Database of Optical Constants -- Level: welcome

... An Orion of a Different Color . ... It is a familiar object though, the grand stellar nursery known as the Orion Nebula . But the striking picture combines images taken through three separate filters, each designed to record different emission lines - light from Sulfur, Oxygen, and Hydrogen atoms glowing in the tenuous nebular gas. At such low densities , Sulfur and Hydrogen atoms emit red colors while Oxygen glows green. ... Publications with keywords: Orion Nebula . ... The Heart Of Orion . ...

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• Астронет > An Orion of a Different Color
• NGC 7129 and NGC 7142
• Journal "Peremennye Zvezdy"