Interpretation of K Emission Line Profile

Proceedings of the Japan Academy
doi 10.2183/pjab1945.42.777
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Japan Academy

Related search

Quasar Emission Line Profile Modelling

Symposium - International Astronomical Union
1989English

X-Ray Emission Line Profile Modeling of Hot Stars

Review of Scientific Instruments
MedicineInstrumentation
2003English

The Origin and Interpretation of Line Profile Variations of Pulsating B Stars

International Astronomical Union Colloquium
2000English

Microlensing in H1413+117: Disentangling Line Profile Emission and Absorption in a Broad Absorption Line Quasar

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2010English

The Origin of K-Shell Emission of Neutral Iron Line From SGR B2

2011English

CARRINGTON MAPS OF Ca II K-Line EMISSION FOR THE YEARS 1915-1985

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2011English

Spatial Population Distribution of Laser Ablation Species Determined by Self-Reversed Emission Line Profile

Journal of Applied Physics
AstronomyPhysics
2002English

Profile of the \(^{12}\)co(3-2) Emission Line Detected From the Debris Disc of 49 Ceti

Communications in Physics
2017English

Quasar Emission - Line Strengths

Symposium - International Astronomical Union
1989English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy