1![X-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](https://www.pdfsearch.io/img/008fc8fd12fafb8af05fbba7af4bcb86.jpg) | Add to Reading ListSource URL: camd.lsu.eduLanguage: English - Date: 2010-12-16 11:54:30
|
---|
2![X-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](https://www.pdfsearch.io/img/d2664df0ed326966a9e5592474ba0bd4.jpg) | Add to Reading ListSource URL: www.camd.lsu.eduLanguage: English - Date: 2010-12-16 11:54:30
|
---|
3![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 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](https://www.pdfsearch.io/img/3640c25c0f8eb433c03fad459f28ee13.jpg) | Add to Reading ListSource URL: www.atomdb.orgLanguage: English - Date: 2014-09-08 21:11:36
|
---|
4![Astronomy & Astrophysics manuscript no. aa25925-15 June 1, 2015 c ESO 2015 Astronomy & Astrophysics manuscript no. aa25925-15 June 1, 2015 c ESO 2015 ](https://www.pdfsearch.io/img/afbfa55faabc5fdbb99e9f79c497544d.jpg) | Add to Reading ListSource URL: cds.aanda.orgLanguage: English |
---|
5![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 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](https://www.pdfsearch.io/img/e5979799c56976ed414b04b189ddaf5c.jpg) | Add to Reading ListSource URL: www.tf.uni-kiel.deLanguage: English - Date: 2015-01-06 05:58:10
|
---|
6![Astronomy & Astrophysics manuscript no. aa25925-15 June 1, 2015 c ESO 2015 Astronomy & Astrophysics manuscript no. aa25925-15 June 1, 2015 c ESO 2015 ](https://www.pdfsearch.io/img/41789101628f1b1ffeb8e01174c2bdbd.jpg) | Add to Reading ListSource URL: www.aanda.orgLanguage: English |
---|
7![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 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](https://www.pdfsearch.io/img/f82435dfa22d928d3eb7637b6e44a7dd.jpg) | Add to Reading ListSource URL: www.atmos-meas-tech-discuss.netLanguage: English - Date: 2015-05-13 08:32:08
|
---|
8![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 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](https://www.pdfsearch.io/img/51fb3e6259b7053a3eaf8d4d1c3dcd4e.jpg) | Add to Reading ListSource URL: www.astrohandbook.comLanguage: English - Date: 2008-12-31 13:13:14
|
---|
9![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 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](https://www.pdfsearch.io/img/fd924d333798a4653803403111ccc784.jpg) | Add to Reading ListSource URL: www.usm.uni-muenchen.deLanguage: English - Date: 2003-06-16 09:14:50
|
---|
10![Astronomy & 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](https://www.pdfsearch.io/img/6c0c2446769cfd3132e44e2fd1a4630c.jpg) | Add to Reading ListSource URL: www.usm.uni-muenchen.deLanguage: English - Date: 2005-02-17 05:00:32
|
---|