Titlebook: B[e] Stars; Anne Marie Hubert,Carlos Jaschek Book 1998 Springer Science+Business Media B.V. 1998 Galaxy.LOPES.galaxies.interferometry.phot

不服從

書目名稱B[e] Stars影響因子(影響力)




書目名稱B[e] Stars影響因子(影響力)學(xué)科排名




書目名稱B[e] Stars網(wǎng)絡(luò)公開度




書目名稱B[e] Stars網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱B[e] Stars被引頻次




書目名稱B[e] Stars被引頻次學(xué)科排名




書目名稱B[e] Stars年度引用




書目名稱B[e] Stars年度引用學(xué)科排名




書目名稱B[e] Stars讀者反饋




書目名稱B[e] Stars讀者反饋學(xué)科排名

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打折

978-90-481-5080-9Springer Science+Business Media B.V. 1998

Highbrow

B[e] Stars978-94-015-9014-3Series ISSN 0067-0057 Series E-ISSN 2214-7985

小故事

cumulative

ACME

muster

The Self Absorption Curve Method for the Analysis of Emission Lines of Complex Ions as a Diagnostic tellar envelope. Information can be obtained notably about the excitation conditions, the column density and the dimensions of the line emitting region, without making detailed model dependent complex radiative transfer computations. This method is particularly useful in the study of B[e] star envelopes.

Alpha-Cells

The High Excitation Fe II Lines as a Diagnostics of the Outer Envelopes of Early Type Emission Line malously high intensities. We illustrate the case of the high excitation Fe . lines observed in the ultraviolet and near—IR of different stellar categories, and discuss the information which can be derived from their study.

杠桿

Rapid Spectral Variability and Spatial and Kinematical Structure of Circumstellar Envelopes of Some tellar envelopes around peculiar Ae/Be stars. The method involved is based on a search for rapid line-profile variability of lines originating in different circumstellar regions. Analysis of these variations opens the way for reconstructing the density and velocity distributions throughout the envelope.