... 000, 000{000 (0000) Printed 1 August 2002 (MN L A T E X style le v2.2) Hydrodynamical simulations of the decay of high-speed molecular turbulence. ... Average Mach number as a function of time; log{log plot. c 0000 RAS, MNRAS 000, 000{000 Simulations of molecular turbulence 5 A rapid power-law decay of kinetic energy with time was uncovered in the isothermal case (Stone et al. ... We carried out three dimensional hy- drodynamical simulations of decaying supersonic turbulence in molecular gas. ...

... July , 2007 . ... 0.12 0.23 +/- 0.10 +/- 0.06 Internal error of single observation 0.18 0.11 ----------------------Compressed Ephemeris DE200/LE200 -------------- MP Obs Dynamical Time RA (O-C)cosDEC DEC (O-C) h m s " ' " " 78756 094 2007 7 22.891513 20 04 27.767 -0.12 - 9 55 57.80 0.32 78756 094 2007 7 22.899703 20 04 27.348 -0.34 - 9 55 58.00 0.30 78756 094 2007 7 22.907823 20 04 26.959 -0.18 - 9 55 58.20 0.28 78756 094 2007 7 22.914753 20 04 26.618 -0.17 - 9 55 58.30 0.33 Mean of last 4 obs. ...

... YES . ... 1.2e+31 . ... 111 . ... 110 . ...

King 13 2.5700 +61.1775 10.0 0.56 0.04 12.36 0.27 2960 400 8.85 0.05 NGC 136 7.8858 +61.5083 4.0 0.70 0.09 13.59 0.14 5220 350 8.40 0.05 Berkeley 19 81.0117 +29.5711 5.0 0.61 0.05 0.72 12.38 0.40 3000 600 9.25 0.05 Czernik 21 81.6708 +36.0136 6.0 0.72 0.02 0.56 11.82 0.20 2300 200 9.55 0.05 Stock 8 82.0367 +34.4314 8.0 1.21 0.04 0.57 9.84 0.20 900 110 7.50 Kronberger 1 82.0917 +34.7733 5.0 0.43 ...

... Column (1): Source name from NED. ... Column (8): Log star formation rate, from SDSS. {\it Detected sources:} (1) (2) (3) (4) (5) (6) (7) IC0159 0.58±0.10 8.31 ± 0.07 8.25 ± 0.07 9.55 9.70 8.89 -0.06 UGC2004 5.98±0.65 9.32 ± 0.04 9.03 ± 0.04 9.83 9.61 9.15 0.36 NGC1234 0.24±0.06 7.92 ± 0.09 7.80 ± 0.09 9.67 9.58 8.98 -0.68 2MASJ0839+03 2.30±0.54 8.91 ± 0.09 8.69 ± 0.09 --- 9.94 9.08 0.58 2MASJ0846+02 2.75±0.47 8.98 ± 0.07 8.85 ± 0.07 --- 9.84 8.99 ...

... bandheads -------------------------------------------------------------------------------- 000705.02+282104.2 52909.37 19.57 0.34 0.14 - 0.06 -0.23 43.5 4.6 -43.6 4.6 000807.54-103405.5 18.93 0.31 0.07 - 0.12 -0.04 20.29 002531.50-110800.8 51792.44 18.00 0.22 0.00 - 0.10 -0.17 19.18 110.7 3.1 -72.2 3.1 010647.93+151327.6 53243.38 19.21 -0.51 -0.35 -0.32 -0.39 -15.1 3.3 -28.7 3.3 010748.20+010240.1 52963.19 18.58 0.55 0.24 0.00 - ...

... Version 0.32 (Marco Beijersbergen) ------------ + recreated with createtestodf-1.2 scisimodf-1.4 scisim_v2.1a19991208 odffix-1.27 Version 0.31 ( JBa ) ------------ + recreated with createtestodf-1.0 scisimodf-1.0 scisim_v2.1.a19991104 odffix-1.26 Version 0.30 (MB) ------------ + recreated with createtestodf-0.23 scisimodf-0.27 scisim_v2.1.a19990917 odffix-1.24 Version 0.29 (MB) ------------ + ... Version 0.6 1998-11-19 ----------- + yet again, we had the wrong names around. ...

Optical and UV Spectrophotometric Standard Stars . ... Two papers detail the observations: the first is devoted to wavelengths from 3300 to 7550A (Hamuy et al., ... -------------------------------------------------------- 718 Xi2 Cet B9 III -O.107 -0.056 4.279 -0.023 -0.063 1544 Pi2 Ori Al V 0.01 4.355 0.014 0.039 3454 Eta Hya B3 V -0.743 -0.200 4.295 -0.083 -0.200 4468 Theta Crt B9.5 V -0.18 -0.07 4.700 -O.023 -0.063 4963 ...

... Printed in U.S.A. Measuring the Balmer Jump and the Effective Gravity in FGK Stars Michael S. Bessell Research School of Astronomy and Astrophysics, Australian National University, Mount Stromlo, Weston, Australia; bessell@mso.anu.edu.au Received 2006 October 17; accepted 2007 May 18; published 2007 June 21 ABSTRACT. ... Synthetic fl spectra for [Fe/H] p 2.5, 5750 K, and log g p 4.5, 3.5, 2.5. ... Synthetic spectra divided by an 11,800 K BB for [Fe/H] p 2.5, 6500 K, and log g p 4.5, 4.0, 2.5. ...

... MICROSCOPES . ... SURGICAL MICROSCOPES . ... Home Products Microscopes Multiscopes EA-Series Achromats and Plan Achromats . EA-SERIES ACHROMATS AND PLAN ACROMATS OBJECTIVES . EA-Series Objectives (Mechanical Tube Length: 160mm; Parfocal Distance: 33mm) . ... Field Flatness . ... EAB Achromats . ... Plan . ... Flat Field . 0.40 . ... Oil Immersion . ... EAP Achromats for Phase Contrast . ... EAF Achromats for Epi-Fluorescence . ... Water Immersion . ...

Next: Access to Data Sources and the ESO SkyCat Tool . ... We describe an implementation of Dynamic Queries (DQ), a recently developed method as an alternative to the perceived complicated SQL-type operations on relational databases by a very intuitive graphical interface. This prototype implementation, written within the NEMO package, uses ASCII sliders and the PGPLOT graphics interface and uses a novel interactive analysis back-end tool that is dynamically associated with the query. ...

... Dust in Nuclei of Galactic Bulges . ... WFPC2 of 20 nuclei of nearby galactic bulges of types S0-Sbc. ... Bulges of spiral galaxies are generally seen as small elliptical galaxies in the center of a large spiral. ... Here we show first results of a color study of the centers of galactic bulges. ... With these three bands we can make the red I - H color, primarily sensitive to extinction by dust and old stellar population gradients, and the B - I color, especially sensitive to recent star formation. ...

The Earth's Orbit . The shape and orientation of the Earth's orbit around the Sun are also changing, under the influence of the other planets. ... The perihelion and aphelion are precessing, advancing eastward along the ecliptic about 11 arcseconds per year in relation to the fixed stars. ... The change in eccentricity, plus the changing relation between the perihelion and aphelion of the Earth's orbit and the equinoxes and solstices, change the duration of the seasons. ...

... Tonight's Sky . ... Observing . ... Star Atlas . ... stars . ... Globular cluster NGC 2808, elliptical galaxy NGC 2986, and the Sextans Dwarf . ... Astronomy for Kids . ... Do brown dwarfs pulsate? ... It's just this temperature sensitivity that should induce pulsations in stars under 0.10 solar mass brown dwarfs and very-low-mass red dwarfs. ... Thus, observers who seek pulsating brown dwarfs should examine groups of young stars, such as those in the constellations of Orion, Taurus, and Chamaeleon....

... METHOD . ... public class GaussianBlur . ... Like all convolution operations in ImageJ, it assumes that out-of-image pixels have a value equal to the nearest edge pixel. ... blur1Direction ( FloatProcessor ip, double sigma, double accuracy, boolean xDirection, int extraLines) . ... convolveLine (float[] input, float[] pixels, float[][] kernel, int readFrom, int readTo, int writeFrom, int writeTo, int point0, int pointInc) . ... makeGaussianKernel (double sigma, double accuracy, int maxRadius) . ...

Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... Irvin M. Winer . ... Weather . ... RainWise Mk III / 100m SW of Observatory . ... RainWise Mk III / N=0 ,E=90 ,S=180 ,W=270 . Air Temperature . ... 0.0 0.36 ( F) . ... AAG IR Sky Temperature . ... AAG Adjusted IR Sky Temperature . ... AAG Ambient Temperature . ... AAG Temperature Split . ... AAG Adjusted Temperature Split . ... Clear Sky Clock for Winer Observatory is provided by Attilla Danko. ... 2013 Winer Observatory. ...

... Planets . ... Stars . Exoplanets . ... Most exoplanets so far discovered fall into the category of тАШhot JupitersтАЩ, these are giant planets orbiting very close to their parent star. ... Note that we have discovered so many hot Jupiters because they are the easiest type of planet to find, they are not necessarily particularly common in the galaxy. ... Subsequently several similar hot and€а fuzzy worlds have been discovered the same way, proving this that this planet is not a one-off oddball. ...

... Home Articles Comet Hyakutake: The Great ?Earthgrazing? Comet of 1996 . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . Observing Resources for Amateur Astronomers - Part 2: Intermediate Observers . ... Comet Hyakutake: The Great "Earthgrazing" Comet of 1996 . A History of the First Forty Years of the Amateur Astronomers Association . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

Apache's support for content negotiation has been updated to meet the HTTP/1.1 specification. It can choose the best representation of a resource based on the browser-supplied preferences for media type, languages, character set and encoding. ... Content-Language: . ... The reason for setting this language quality factor for variant with no language to a very low value is to allow for a default variant which can be supplied if none of the other variants match the browser's language preferences. ...