On the spectrum of a gaseous nebula of pure hydrogen - III: The Balmer decrement
The Balmer decrement was calculated for a homogeneous, spherical, pure hydrogen nebula, ionised and excited both by radiative and collisional processes. Reabsorption in the Balmer series from sublevels 2 s and 2 p was taken into account. Calculations were carried out for electron temperatures of 104...
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todo:paper_0004640X_v10_n3_p383_Gerola2023-10-03T14:02:46Z On the spectrum of a gaseous nebula of pure hydrogen - III: The Balmer decrement Gerola, H. Salem, M. Panagia, N. The Balmer decrement was calculated for a homogeneous, spherical, pure hydrogen nebula, ionised and excited both by radiative and collisional processes. Reabsorption in the Balmer series from sublevels 2 s and 2 p was taken into account. Calculations were carried out for electron temperatures of 104 K and 2×104 K, electron densities from 103 to 106 cm-3, and radii from 1015 to 1017 cm. The results define allowed and forbidden regions in the log(Hβ/Hγ) vs log(Hα/Hβ) diagram different from those of previous results obtained assuming purely radiative or purely collisional ionisation and excitation. A brief comparison with observations is presented and discussed. © 1971 D. Reidel Publishing Company. Fil:Salem, M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0004640X_v10_n3_p383_Gerola |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
description |
The Balmer decrement was calculated for a homogeneous, spherical, pure hydrogen nebula, ionised and excited both by radiative and collisional processes. Reabsorption in the Balmer series from sublevels 2 s and 2 p was taken into account. Calculations were carried out for electron temperatures of 104 K and 2×104 K, electron densities from 103 to 106 cm-3, and radii from 1015 to 1017 cm. The results define allowed and forbidden regions in the log(Hβ/Hγ) vs log(Hα/Hβ) diagram different from those of previous results obtained assuming purely radiative or purely collisional ionisation and excitation. A brief comparison with observations is presented and discussed. © 1971 D. Reidel Publishing Company. |
format |
JOUR |
author |
Gerola, H. Salem, M. Panagia, N. |
spellingShingle |
Gerola, H. Salem, M. Panagia, N. On the spectrum of a gaseous nebula of pure hydrogen - III: The Balmer decrement |
author_facet |
Gerola, H. Salem, M. Panagia, N. |
author_sort |
Gerola, H. |
title |
On the spectrum of a gaseous nebula of pure hydrogen - III: The Balmer decrement |
title_short |
On the spectrum of a gaseous nebula of pure hydrogen - III: The Balmer decrement |
title_full |
On the spectrum of a gaseous nebula of pure hydrogen - III: The Balmer decrement |
title_fullStr |
On the spectrum of a gaseous nebula of pure hydrogen - III: The Balmer decrement |
title_full_unstemmed |
On the spectrum of a gaseous nebula of pure hydrogen - III: The Balmer decrement |
title_sort |
on the spectrum of a gaseous nebula of pure hydrogen - iii: the balmer decrement |
url |
http://hdl.handle.net/20.500.12110/paper_0004640X_v10_n3_p383_Gerola |
work_keys_str_mv |
AT gerolah onthespectrumofagaseousnebulaofpurehydrogeniiithebalmerdecrement AT salemm onthespectrumofagaseousnebulaofpurehydrogeniiithebalmerdecrement AT panagian onthespectrumofagaseousnebulaofpurehydrogeniiithebalmerdecrement |
_version_ |
1782028367340503040 |