Add to ORKGAstronomical models of galactic nuclei emission spectra are reassessed in light of ultraviolet and X-ray spectroscopic observations. Spectral analysis of BL Lacertae objects using data collected by the International Ultraviolet Explorer (IUE) and other astronomical observatories is presented
The results of the 9th and 10th IUE episode programs listed are summarized. Observations and basic d...
Active galaxies are most luminous objects in the universe whose spectra are characterized by both pe...
We compute synthetic optical and ultraviolet (UV) emission-line properties of galaxies in a full cos...
The status of research undertaken with the IUE satellite for programs on strong binary X-ray stars a...
Ultraviolet studies of astronomical sources are discussed. Some studies utilized IVE data. Non-radia...
The IUE observations of four active nuclei were coordinated with radio, infrared, and X-ray measurem...
A review of the field of astronomical spectroscopy with emphasis on emission lines in astrophysical ...
The observation, data reduction, and interpretation of ultraviolet spectra (obtained with the Intern...
Ultraviolet spectra of bright Seyfert 1 galaxies will be obtained with the Hubble Space Telescope. O...
The spectra of active galactic nuclei (AGNs) are important probes of astrophysical phenomena on many...
International audienceWe compute synthetic optical and ultraviolet (UV) emission-line properties of ...
The IUE satellite observatory was used to obtain absolutely-calibrated emission line fluxes for diag...
No new International Ultraviolet Explorer (IUE) observations were scheduled. The work on the spectra...
© 2020 by the authors.This paper reviews several basic emission properties of the UV emission lines ...
The ionizing continuum from active galactic nuclei is fundamental for interpreting their broad emiss...
The results of the 9th and 10th IUE episode programs listed are summarized. Observations and basic d...
Active galaxies are most luminous objects in the universe whose spectra are characterized by both pe...
We compute synthetic optical and ultraviolet (UV) emission-line properties of galaxies in a full cos...
The status of research undertaken with the IUE satellite for programs on strong binary X-ray stars a...
Ultraviolet studies of astronomical sources are discussed. Some studies utilized IVE data. Non-radia...
The IUE observations of four active nuclei were coordinated with radio, infrared, and X-ray measurem...
A review of the field of astronomical spectroscopy with emphasis on emission lines in astrophysical ...
The observation, data reduction, and interpretation of ultraviolet spectra (obtained with the Intern...
Ultraviolet spectra of bright Seyfert 1 galaxies will be obtained with the Hubble Space Telescope. O...
The spectra of active galactic nuclei (AGNs) are important probes of astrophysical phenomena on many...
International audienceWe compute synthetic optical and ultraviolet (UV) emission-line properties of ...
The IUE satellite observatory was used to obtain absolutely-calibrated emission line fluxes for diag...
No new International Ultraviolet Explorer (IUE) observations were scheduled. The work on the spectra...
© 2020 by the authors.This paper reviews several basic emission properties of the UV emission lines ...
The ionizing continuum from active galactic nuclei is fundamental for interpreting their broad emiss...
The results of the 9th and 10th IUE episode programs listed are summarized. Observations and basic d...
Active galaxies are most luminous objects in the universe whose spectra are characterized by both pe...
We compute synthetic optical and ultraviolet (UV) emission-line properties of galaxies in a full cos...