1![Searching for Interstellar Archaeology signatures with Dyson Spheres on the stellar and galactic scale Dick Carriganwith help from Nancy Carrigan Searching for Interstellar Archaeology signatures with Dyson Spheres on the stellar and galactic scale Dick Carriganwith help from Nancy Carrigan](https://www.pdfsearch.io/img/f6ae361d124b2bdc1dd6bd0ff6738707.jpg) | Add to Reading ListSource URL: home.fnal.govLanguage: English - Date: 2015-11-16 15:40:49
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2![The universe in a cup of coffee John S. Wettlaufer Your morning java or tea is a rotating, cooling laboratory that reflects the physics of such large-scale phenomena as stellar dynamics and energy transport in Earth’s The universe in a cup of coffee John S. Wettlaufer Your morning java or tea is a rotating, cooling laboratory that reflects the physics of such large-scale phenomena as stellar dynamics and energy transport in Earth’s](https://www.pdfsearch.io/img/dd2d608554867b9b63f76dbbd039f37f.jpg) | Add to Reading ListSource URL: www.pmc.ucsc.eduLanguage: English - Date: 2012-01-21 17:40:03
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3![Challenges
in
opacity
modeling
for
planetary
and
stellar
atmosphere
studies:
line
widths
R.E.Lupu1,
R.S.Freedman1,
and
M.S.Marley2
1.SETI
InsCtu Challenges
in
opacity
modeling
for
planetary
and
stellar
atmosphere
studies:
line
widths
R.E.Lupu1,
R.S.Freedman1,
and
M.S.Marley2
1.SETI
InsCtu](https://www.pdfsearch.io/img/3d35ea0f6f204463e60b67e3997d9719.jpg) | Add to Reading ListSource URL: www.astro.ex.ac.ukLanguage: English - Date: 2012-02-06 09:02:04
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4![1 CHAPTER 5 ABSORPTION, SCATTERING, EXTINCTION AND THE EQUATION OF TRANSFER 5.1 Introduction As radiation struggles to make its way upwards through a stellar atmosphere, it may be 1 CHAPTER 5 ABSORPTION, SCATTERING, EXTINCTION AND THE EQUATION OF TRANSFER 5.1 Introduction As radiation struggles to make its way upwards through a stellar atmosphere, it may be](https://www.pdfsearch.io/img/d9aaa1e782726d4aa5b70d5684810c8c.jpg) | Add to Reading ListSource URL: astrowww.phys.uvic.caLanguage: English - Date: 2006-04-12 19:06:23
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5![Click Here JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 113, E00B23, doi:2008JE003140, 2008 for Click Here JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 113, E00B23, doi:2008JE003140, 2008 for](https://www.pdfsearch.io/img/941c953286bead11135c8013bf11416f.jpg) | Add to Reading ListSource URL: venus.aeronomie.beLanguage: English - Date: 2009-07-10 10:51:52
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6![Click Here JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 113, E00B23, doi:2008JE003140, 2008 for Click Here JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 113, E00B23, doi:2008JE003140, 2008 for](https://www.pdfsearch.io/img/d0de27cdf9f7e9e057f5e8426f7c0fed.jpg) | Add to Reading ListSource URL: planetary.aeronomie.beLanguage: English - Date: 2009-07-10 10:51:52
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7![Question 5. (a) Suppose the Local Thermodynamic Equilibrium assumption holds for the stellar atmosphere. Prove that for the optically thin line, the absorption line depth R can be written as R where
Question 5. (a) Suppose the Local Thermodynamic Equilibrium assumption holds for the stellar atmosphere. Prove that for the optically thin line, the absorption line depth R can be written as R where](https://www.pdfsearch.io/img/ccb4a6c17551dd4883fb7da7b8ba5987.jpg) | Add to Reading ListSource URL: www.astro.ncu.edu.twLanguage: English - Date: 2014-05-12 00:06:46
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8![Institute of Astronomy, National Central University PHD QUALIFYING EXAMINATION — STELLAR ASTROPHYSICS 26th May, points) A stellar atmosphere in which the opacity is assumed to be independent of wavelength Institute of Astronomy, National Central University PHD QUALIFYING EXAMINATION — STELLAR ASTROPHYSICS 26th May, points) A stellar atmosphere in which the opacity is assumed to be independent of wavelength](https://www.pdfsearch.io/img/1b2ea445b45fa168538219980a58ca13.jpg) | Add to Reading ListSource URL: www.astro.ncu.edu.twLanguage: English - Date: 2014-05-12 00:06:46
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9![1 CHAPTER 5 ABSORPTION, SCATTERING, EXTINCTION AND THE EQUATION OF TRANSFER 5.1 Introduction As radiation struggles to make its way upwards through a stellar atmosphere, it may be 1 CHAPTER 5 ABSORPTION, SCATTERING, EXTINCTION AND THE EQUATION OF TRANSFER 5.1 Introduction As radiation struggles to make its way upwards through a stellar atmosphere, it may be](https://www.pdfsearch.io/img/8200f55a6ebe3ce000a5d77a196f2a6c.jpg) | Add to Reading ListSource URL: orca.phys.uvic.caLanguage: English - Date: 2006-04-12 19:06:23
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10![Bern Lectures 2014: Photoevaporation Photolysis and photoevaporation Raymond T. Pierrehumbert The University of Chicago Bern Lectures 2014: Photoevaporation Photolysis and photoevaporation Raymond T. Pierrehumbert The University of Chicago](https://www.pdfsearch.io/img/57b67e3c56d7ebbf849918925731b308.jpg) | Add to Reading ListSource URL: www.csh.unibe.chLanguage: English - Date: 2014-02-25 05:41:31
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