We have discovered polarized broad emission lines in five type 2 Seyfert galaxies (NGC 424, NGC 591, NGC 2273, NGC 3081, and NGC 4507), establishing that these objects are type 1 Seyferts obscured by dense circumnuclear material. The galaxies are part of a distance-limited sample of 31 Seyfert 2s, for which spectropolarimetric observations are now complete. Combined with published reports, our results indicate that at least 11 of the galaxies in this sample, or > 35%, possess hidden broad-line regions. This represents the first reliable estimate of the frequency of polarized broad emission lines in type 2 Seyferts, which has important implications for the general applicability of Seyfert unification models
We formulate a perturbative approximation to gravitational instability, based on Lagrangian hydrodyn...
A class of structural time series models with an asymmetric cyclical component is presented and used...
I describe the current status of tests of perturbative QCD, using measurements of jet, photon, weak ...
Future space and ground-based survey programmes will produce an impressiveamount of photometric data...
One hundred years after the eruption of GK Per and the detection of oscillations in its light curve ...
In economic models, it is usually assumed that agents aggregate their private and all available publ...
We consider a model of international migration with heterogeneity in the skill level of workers whic...
Given a probability density f on R^d, the minimum volume set of probability content á can be estimat...
Gravitational microlensing at cosmological distances is potentially a powerful tool for probing the ...
Two studies have recently reported the discovery of pronounced Halo substructure in the Sloan Digita...
We demonstrate that the Biermann battery mechanism for the creation of large scale magnetic fields c...
About 500d after explosion the light curve of the Type Ia SN1998bu suddenly flattened and at the sam...
We study the generation and maintenance of large-scale magnetic fields in barred galaxies. We take a...
At OAB we were, during the year 1998, deeply involved in planning two important space missions for w...
Although soft X-ray absorption features in AGN were discovered almost ten years ago, the nature and ...
We formulate a perturbative approximation to gravitational instability, based on Lagrangian hydrodyn...
A class of structural time series models with an asymmetric cyclical component is presented and used...
I describe the current status of tests of perturbative QCD, using measurements of jet, photon, weak ...
Future space and ground-based survey programmes will produce an impressiveamount of photometric data...
One hundred years after the eruption of GK Per and the detection of oscillations in its light curve ...
In economic models, it is usually assumed that agents aggregate their private and all available publ...
We consider a model of international migration with heterogeneity in the skill level of workers whic...
Given a probability density f on R^d, the minimum volume set of probability content á can be estimat...
Gravitational microlensing at cosmological distances is potentially a powerful tool for probing the ...
Two studies have recently reported the discovery of pronounced Halo substructure in the Sloan Digita...
We demonstrate that the Biermann battery mechanism for the creation of large scale magnetic fields c...
About 500d after explosion the light curve of the Type Ia SN1998bu suddenly flattened and at the sam...
We study the generation and maintenance of large-scale magnetic fields in barred galaxies. We take a...
At OAB we were, during the year 1998, deeply involved in planning two important space missions for w...
Although soft X-ray absorption features in AGN were discovered almost ten years ago, the nature and ...
We formulate a perturbative approximation to gravitational instability, based on Lagrangian hydrodyn...
A class of structural time series models with an asymmetric cyclical component is presented and used...
I describe the current status of tests of perturbative QCD, using measurements of jet, photon, weak ...