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1. The Local Volume HI Survey (LVHIS)
The Australia Telescope Compact Array (ATCA) . Home page Team Galaxy Sample Observations Papers Projects Related Surveys Pipeline Meetings . Local Volume galaxies ( B. Koribalski) . The Local Volume HI Survey'' (LVHIS) is a project comprising deep HI line and 20-cm radio continuum observations for all nearby, gas-rich galaxies, supplemented by multi-wavelength data. ... Our aim is to study the formation and evolution of galaxies in the Local Universe. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/bkoribal/LVHIS/ -- 7.0 Кб -- 10.04.2016
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2. http://www.arcetri.astro.it/radtran/talks/cvlahakis.pdf
The SCUBA Local Universe Galaxy Survey Dust along the Hubble sequence Catherine Vlahakis University of Bonn Collaborators: Steve Eales (Cardiff University) Loretta Dunne (University of Nottingham) Overview What is SLUGS? Results from the survey Recent work using SLUGS results ­ the FIR-radio relation Introduction: SLUGS SLUGS ­ a submm survey of galaxies in the local Universe ­ at 850m and 450m Survey of ~200 nearby galaxies: 104 60m-selected ("IRS") (Dunne et al. ...
[ Текст ]  Ссылки http://www.arcetri.astro.it/radtran/talks/cvlahakis.pdf -- 460.3 Кб -- 25.06.2007
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3. The State of the Gas and the Relation between Gas and Star Formation at Low
We compare atomic gas, molecular gas, and the recent star formation rate (SFR) inferred from HЮБ in the Small Magellanic Cloud (SMC). ... This allows us to disentangle conversion factor effects from the impact of metallicity on the formation and star formation efficiency of molecular gas. ... At a fixed total gas surface density the SMC has a 5-10 times lower molecular gas fraction (and star formation rate) than large spiral galaxies. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2011ApJ...741...12B.html -- 5.5 Кб -- 21.01.2016
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4. Gimp related links collection
... Now I have an occasion - Grokking the GIMP by Carey Bunks ! ... I have Linux binaries gimp-1.0.2.linux.tgz of current development version with all patches applied and plugins updated . ... I used to configure gimp with --prefix=/usr/local/gimp, so everything will go to /usr/local/gimp directory. Just make a symbolic link to make it visible ( e.g. ln -s /usr/local/gimp/bin/gimp /usr/local/bin/gimp). ... Also, you need gtk libraries installed ! ... GIMP Plugin Registry . ... figures plugin . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~megera/gimp/ -- 13.5 Кб -- 21.12.2007
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5. Common Holidays in Relation to Equinoxes, Solstices Cross-Quarter Days
... The Cross-Quarter Days thus mark the middle of each season under our current system, or seasonal boundaries under the alternative system. ... Beltane / Bealtaine - Celtic bonfire festival May 4-7 2nd Cross-Quarter Day May 5 - Cinco de Mayo (Mexico) May 2nd Sunday - Mother's Day May last Monday - Memorial Day ( Decoration Day , officially May 30) June 14 - Flag Day June 3rd Sunday - Father's Day June 20-22 2nd Quarter Day - Summer Solstice June 21 - Litha (Norse/Anglo-Saxon for ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~gibson/cal/ -- 18.8 Кб -- 18.11.2010
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6. Dispersion relation [Oulu]
... All the information about the propagation of a given plasma wave mode is contained in the appropriate dispersion relation, which relates the angular frequency w to the wave number k (magnitude of the propagation vector k ). ... Phase velocity . ... Group velocity . ... Wave propagation can also be described using diagrams called phase velocity or wave normal surfaces , which give the variations of the magnitude of the phase velocity of plane waves with respect to the magnetic field direction: . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/disprel.html -- 4.4 Кб -- 21.12.2007
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7. Relations
... Mindful of these biases, I can now explore the relations between the measured rotation periods and various other observables. The hypothesis behind monitoring stellar variability is that active stars have asymmetric spot distributions on their photospheres. ... They found that only stars with rotation periods greater than seven days show variations greater than 0.4 magnitudes at I. Bouvier et al . ... 1993a) demonstrated a relation between X--ray flux and spectral type in ZAMS stars. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~swolk/thesis/discussion/node3.html -- 7.2 Кб -- 02.10.2012
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