Atomic spectral line

Results: 63



#Item
1X-Ray Data Booklet Table 1-2. Photon energies, in electron volts, of principal K-, L-, and M-shell emission lines. Element

X-Ray Data Booklet Table 1-2. Photon energies, in electron volts, of principal K-, L-, and M-shell emission lines. Element

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Source URL: camd.lsu.edu

Language: English - Date: 2010-12-16 11:54:30
2X-Ray Data Booklet Table 1-2. Photon energies, in electron volts, of principal K-, L-, and M-shell emission lines. Element

X-Ray Data Booklet Table 1-2. Photon energies, in electron volts, of principal K-, L-, and M-shell emission lines. Element

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Source URL: www.camd.lsu.edu

Language: English - Date: 2010-12-16 11:54:30
3Study of the resonant scattering in the Perseus cluster core with ASTRO-H Saori Konami (Tokyo Metropolitan University) Irina Zhuravleva (Stanford Univ.), Eugene Churazov, Rashid Sunyaev (MPA) Kosuke Sato (Tokyo Univ. of

Study of the resonant scattering in the Perseus cluster core with ASTRO-H Saori Konami (Tokyo Metropolitan University) Irina Zhuravleva (Stanford Univ.), Eugene Churazov, Rashid Sunyaev (MPA) Kosuke Sato (Tokyo Univ. of

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Source URL: www.atomdb.org

Language: English - Date: 2014-09-08 21:11:36
4Astronomy & Astrophysics manuscript no. aa25925-15 June 1, 2015 c ESO 2015 

Astronomy & Astrophysics manuscript no. aa25925-15 June 1, 2015 c ESO 2015 

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Source URL: cds.aanda.org

Language: English
5Einstein Coefficients Again, we come back to the question: Do (direct) semiconductors glow in the dark? The answer was yes – but only to the extent that all (black) bodies glow in the dark, following Plancks famous for

Einstein Coefficients Again, we come back to the question: Do (direct) semiconductors glow in the dark? The answer was yes – but only to the extent that all (black) bodies glow in the dark, following Plancks famous for

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Source URL: www.tf.uni-kiel.de

Language: English - Date: 2015-01-06 05:58:10
6Astronomy & Astrophysics manuscript no. aa25925-15 June 1, 2015 c ESO 2015 

Astronomy & Astrophysics manuscript no. aa25925-15 June 1, 2015 c ESO 2015 

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Source URL: www.aanda.org

Language: English
7Supplement of Atmos. Meas. Tech. Discuss., 8, 4859–4916, 2015 http://www.atmos-meas-tech-discuss.netdoi:amtdsupplement © Author(sCC Attribution 3.0 License. Supplement of

Supplement of Atmos. Meas. Tech. Discuss., 8, 4859–4916, 2015 http://www.atmos-meas-tech-discuss.netdoi:amtdsupplement © Author(sCC Attribution 3.0 License. Supplement of

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Source URL: www.atmos-meas-tech-discuss.net

Language: English - Date: 2015-05-13 08:32:08
8ATOMIC SPECTROSCOPY Spectroscopic notation combines observational and theoretical elements. Observationally, spectral lines are grouped in series with line spacings which decrease toward the series limit. Every line can

ATOMIC SPECTROSCOPY Spectroscopic notation combines observational and theoretical elements. Observationally, spectral lines are grouped in series with line spacings which decrease toward the series limit. Every line can

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Source URL: www.astrohandbook.com

Language: English - Date: 2008-12-31 13:13:14
9Astronomy & Astrophysics manuscript no. (will be inserted by hand later) Radiation-driven winds of hot luminous stars XIII. A description of NLTE line blocking and blanketing towards realistic models for expanding atmosp

Astronomy & Astrophysics manuscript no. (will be inserted by hand later) Radiation-driven winds of hot luminous stars XIII. A description of NLTE line blocking and blanketing towards realistic models for expanding atmosp

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Source URL: www.usm.uni-muenchen.de

Language: English - Date: 2003-06-16 09:14:50
10Astronomy & Astrophysics manuscript no. paper (DOI: will be inserted by hand later) February 17, 2005 Atmospheric NLTE-models for the spectroscopic analysis of blue

Astronomy & Astrophysics manuscript no. paper (DOI: will be inserted by hand later) February 17, 2005 Atmospheric NLTE-models for the spectroscopic analysis of blue

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Source URL: www.usm.uni-muenchen.de

Language: English - Date: 2005-02-17 05:00:32