Results 31 to 40 of about 344,061 (314)

SPECTRAL AND PHOTOMETRIC STUDIES OF MRK6 AND MRK1040 IN THE OPTICAL RANGE

open access: yesEurasian Physical Technical Journal
This paper is dedicated to the study of variability in active galactic nuclei, which play a key role in understanding the physical processes occurring in their central regions.
S.A. Shomshekova   +5 more
doaj   +1 more source

News from AG Draconis

open access: yesOpen Astronomy, 2012
AG Dra is a classical symbiotic star that undergoes major outbursts at intervals between 12-15 years. We present spectroscopic observations of four emission lines (Hα, Hβ, He II 4686 Å, Raman scattered OVI 6825 Å) before, during and after the major ...
Leedjärv L., Burmeister M.
doaj   +1 more source

Exploring Possible Relations Between Optical Variability Time Scales and Broad Emission Line Shapes in AGN

open access: yesFrontiers in Astronomy and Space Sciences, 2018
Here we investigate the connection of broad emission line shapes and continuum light curve variability time scales of type-1 Active Galactic Nuclei (AGN).
Edi Bon   +4 more
doaj   +1 more source

Spectral and Photometric Studies of NGC 7469 in the Optical Range

open access: yesUniverse
The galaxy NGC 7469 is a bright infrared source with an active galactic nucleus (AGN) and an intense star-forming region with a radius of approximately 500 parsecs, where the star formation rate is estimated to be 20–50 M⊙yr−1.
Saule Shomshekova   +5 more
doaj   +1 more source

Hints on the Broad Line Region Structure of Quasars at High and Low Luminosities

open access: yesOpen Astronomy, 2011
Quasars show a considerable spectroscopic diversity. However, the variety of quasar spectra at low redshifts is non-random: a principal component analysis applied to large samples customarily identifies two main eigenvectors. In this contribution we show
Marziani Paola   +4 more
doaj   +1 more source

Self-Consistent Dynamical Model of the Broad Line Region

open access: yesFrontiers in Astronomy and Space Sciences, 2017
We develop a self-consistent description of the Broad Line Region based on the concept of a failed wind powered by radiation pressure acting on a dusty accretion disk atmosphere in Keplerian motion. The material raised high above the disk is illuminated,
Bozena Czerny   +7 more
doaj   +1 more source

Interpreting broad emission-line variations – I. Factors influencing the emission-line response [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2014
21 pages, 17 figures, accepted for publication in MNRAS July ...
Goad, Michael R., Korista, K. T.
openaire   +3 more sources

[89Zr]Oxinate4 for long-term in vivo cell tracking by positron emission tomography [PDF]

open access: yes, 2014
Purpose 111In (typically as [111In]oxinate3) is a gold standard radiolabel for cell tracking in humans by scintigraphy. A long half-life positron-emitting radiolabel to serve the same purpose using positron emission tomography (PET) has long been ...
Meszaros, L.K.   +26 more
core   +1 more source

Investigation of the Nature of the B[e] Star CI Cam in the Optical Range

open access: yesGalaxies
The B[e] phenomenon is observed in a wide range of stars at various evolutionary stages. Its nature remains uncertain. The B[e] phenomenon is defined as the simultaneous presence of low-excitation forbidden line emission and strong infrared excess in the
Elena A. Barsukova   +3 more
doaj   +1 more source

High Redshift Quasars, Emission Lines and ‘Cloudy’

open access: yesOpen Astronomy, 2011
I describe some of the outstanding “big picture” questions in quasar research and how the development of the plasma simulation code Cloudy is being guided to answer them.
Ferland Gary J.
doaj   +1 more source

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