Content About: Astrophysics
Joint Institute for Laboratory Astrophysics of the National Bureau of Standards and the University of Colorado (Observatory Report)
Towards optimal measurement of power spectra - II. A basis of positive, compact, statistically orthogonal kernels
Variable C IV Absorption in the Seyfert Galaxy NGC 5548: A Connection to Broad Absorption Line Quasi-stellar Objects?
The effects of X-rays from active galactic nuclei on the interstellar medium of the surrounding galaxy
Visualizing the three-dimensional structure of the local interstellar medium and possible physical causes for this structure
Simultaneous Hubble Space Telescope and ASCA Observations of LMC X‐4: X‐Ray Ionization Effects on a Stellar Wind
Total Recombination and Energy Loss Coefficients for Hydrogenic Ions at Low Density for 10<T/E/Z/2<10/7K
Observed and Computed Stellar Line Profiles: The Roles Played by Partial Redistribution, Geometrical Extent and Expansion
A Non-LTE Analysis of the zeta Aurigae B-Type Secondary. I. Determination of the Fundamental Stellar Parameters
X-ray sources in regions of star formation. III - Naked T Tauri stars associated with the Taurus-Auriga complex
Published: 10/19/2012 - 11:38am Type of Content: People - Faculty & Research Groups
Erratum: "Evidence for a corona of Beta Geminorum" [Astrophys. J., Lett., Vol. 193, p. L107 - L110 (1974)].
The relation between the visual polarisation and UV narrow absorption lines in irregular Be star variations