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  • ==Theory of regions== ...f [[geography]], studied by [[w:Regional geography|regional geographers]]. Regions consist of [[w:subregions|subregions]] that contain clusters of like areas ...
    22 KB (3,213 words) - 02:22, 1 December 2020
  • '''The content of these notes is based on the lectures by [http://www.math.utah.edu/~milton/ Prof. Graeme W. Milton] (University o Let the interface between regions 1 and 2 be located at <math>z = -d_1</math> and ...
    10 KB (1,677 words) - 03:02, 7 September 2011
  • ...ud|Large Magellanic Cloud]]. It is one of the largest known star formation regions anywhere.]] ...atistical data, for example demographic, and locales. In astrophysics some regions have science-specific terms such as galactic clusters."<ref name=Region>{{ ...
    20 KB (2,975 words) - 08:13, 11 January 2022
  • '''The content of these notes is based on the lectures by [http://www.math.utah.edu/~milton/ Prof. Graeme W. Milton] (University o The medium consists of three layers. Regions 1 and 3 are isotropic while ...
    18 KB (2,873 words) - 03:03, 7 September 2011
  • ...|thumb|right|250px|A ray trace through a prism with apex angle α is shown. Regions 0, 1, and 2 have indices of refraction <math>n_0</math>, <math>n_1</math>, [[Category:Astrophysics/Lectures]] ...
    11 KB (1,585 words) - 21:00, 12 April 2023
  • |title=Gas in the Central Regions of AGN: The Interstellar Medium and Supermassive Gaseous Objects, In: ''The ...uires] that they are not primarily magnetically supported in their central regions."<ref name=Pringle/> ...
    14 KB (2,101 words) - 19:34, 26 August 2022
  • ==Star-forming regions== {{main|Stars/Star-forming regions|Star-forming regions}} ...
    18 KB (2,848 words) - 23:51, 29 April 2020
  • '''The content of these notes is based on the lectures by [http://www.math.utah.edu/~milton/ Prof. Graeme W. Milton] (University o |[[image:WKBProfile.jpg|thumb|400px|Figure 3. Regions of validity of the linear solution and the WKB solution for large <math>\om ...
    16 KB (2,603 words) - 21:48, 6 March 2022
  • '''The content of these notes is based on the lectures by [http://www.math.utah.edu/~milton/ Prof. Graeme W. Milton] (University o alternating bands of dark and light regions in some cases. An example of ...
    16 KB (2,723 words) - 08:15, 27 April 2024
  • '''The content of these notes is based on the lectures by [http://www.math.utah.edu/~milton/ Prof. Graeme W. Milton] (University o time in such regions as the loss <math>\delta \rightarrow 0</math>. This is clearly ...
    16 KB (2,288 words) - 03:06, 7 September 2011
  • ...6650|bibcode = 1981Sci...211..700W }}</ref> Faculae in magnetically active regions are hotter and 'brighter' than the average photosphere and cause temporary ...lves are darker, they form when there are particularly magnetically active regions, which is when larger, brighter, longer-duration Faculae are more common as ...
    32 KB (4,802 words) - 09:48, 30 May 2023
  • ...Hα Interferometric Optical and Near IR Photometric Studies of Star Forming Regions I. The Cepheus-B/Sh2-155/Cepheus OB3 association complex [[Category:Radiation astronomy/Lectures]] ...
    19 KB (2,727 words) - 07:40, 31 December 2021
  • In the model shown at right the Sun and regions around it are labeled. ==Transition regions== ...
    38 KB (5,855 words) - 09:48, 30 May 2023
  • '''The content of these notes is based on the lectures by [http://www.math.utah.edu/~milton/ Prof. Graeme W. Milton] (University o all such regions of analyticity, we conclude that <math>\boldsymbol{\epsilon}_\text{eff}</ma ...
    20 KB (2,789 words) - 03:06, 7 September 2011
  • '''The content of these notes is based on the lectures by [http://www.math.utah.edu/~milton/ Prof. Graeme W. Milton] (University o ...f, there is interference between preceding and succeeding wavefronts. The regions of constructive and destructive interference give rise to supernumerary ban ...
    12 KB (2,059 words) - 16:34, 25 February 2018
  • ...[logic]] (the trivium), along with [[arithmetic]], [[geometry]], [[Keynote lectures/Astronomy|astronomy]] and [[School:Music and Dance|music]] (the quadrivium) ==Regions== ...
    43 KB (5,978 words) - 02:21, 1 December 2020
  • These "ionization cones" are "conical regions of high-excitation emission-line gas extending from an active nucleus. ... [[Category:Radiation astronomy/Lectures]] ...
    14 KB (2,136 words) - 23:15, 14 November 2022
  • |title=Space Technology 5 observations of the imbalance of regions 1 and 2 field-aligned currents and its implication to the cross-polar cap P * [[Keynote lectures/Astrophysics|Astrophysics]] (106 kB) (7 July 2019‎) ...
    26 KB (4,032 words) - 16:31, 29 November 2020
  • ==Transition regions== {{main|Stars/Transition regions|Transition regions}} ...
    46 KB (6,808 words) - 21:49, 30 November 2020
  • H I regions are non-luminous, save for emission of the hydrogen line at 21-cm (1,420 MH ...— the raw materials for new stars. The many young stars that form in these regions make the spiral arms appear bright and bluish."<ref name=Claude>{{ cite boo ...
    38 KB (5,964 words) - 05:18, 18 December 2019
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