Broad Absorption Line Quasars (BAL QSOs) have been found to be associated with extremely compact radio sources. These reduced dimensions can be either due to projection effects or these objects might actually be intrinsically small. Exploring these two hypotheses is important to understand the nature and origin of the BAL phenomenon because orientation effects are an important discriminant between the different models proposed to explain this phenomenon. In this work we present VLBA observations of 5 BAL QSOs and discuss their pc-scale morphology
Multi-frequency 1.7, 5 and 8.4-GHz VLBA observations of a radio-loud broad absorption line (BAL) qua...
Abstract Broad Absorption Lines (BALs) seem to be the most extreme manifestations of quasar (QSO) ou...
We propose a morphological classification based on the parsec scale structure of fifty-one High Freq...
Broad Absorption Line Quasars (BAL QSOs) have been found to be associated with extremely compact rad...
Context. Broad absorption line quasars (BAL QSOs) belong to a class of objects not well-understood a...
Context. Broad absorption line quasars (BAL QSOs) belong to a class of objects not well-understood a...
Abstract. For a long time, radio-loud Broad Absorption Line Quasars (BAL QSOs) were thought to be ex...
Aims. Outflows manifest as broad absorption lines (BALs) in the quasars spectra. Although outflows a...
ABSTRACT: BAL QSOs are still a not-well understood class of objects. In the UV spectra they show Bro...
We present the results of EVN+MERLIN very long baseline interferometry (VLBI) polarization observati...
Aims.Multifrequency VLBA observations of the final group of ten objects in a sample of FIRST-based ...
none9siAccounting for ∼20% of the total QSO population, Broad Absorption Line QSOs are still an unso...
We report the discovery of five broad-absorption-line (BAL) QSOs in a complete sample of 111 ultravi...
We present the results of European VLBI Network observations of 3 Broad Absorption Line quasars at ...
Context. Broad absorption lines (BALs) are present in the spectra of ~20% of quasars (QSOs); this in...
Multi-frequency 1.7, 5 and 8.4-GHz VLBA observations of a radio-loud broad absorption line (BAL) qua...
Abstract Broad Absorption Lines (BALs) seem to be the most extreme manifestations of quasar (QSO) ou...
We propose a morphological classification based on the parsec scale structure of fifty-one High Freq...
Broad Absorption Line Quasars (BAL QSOs) have been found to be associated with extremely compact rad...
Context. Broad absorption line quasars (BAL QSOs) belong to a class of objects not well-understood a...
Context. Broad absorption line quasars (BAL QSOs) belong to a class of objects not well-understood a...
Abstract. For a long time, radio-loud Broad Absorption Line Quasars (BAL QSOs) were thought to be ex...
Aims. Outflows manifest as broad absorption lines (BALs) in the quasars spectra. Although outflows a...
ABSTRACT: BAL QSOs are still a not-well understood class of objects. In the UV spectra they show Bro...
We present the results of EVN+MERLIN very long baseline interferometry (VLBI) polarization observati...
Aims.Multifrequency VLBA observations of the final group of ten objects in a sample of FIRST-based ...
none9siAccounting for ∼20% of the total QSO population, Broad Absorption Line QSOs are still an unso...
We report the discovery of five broad-absorption-line (BAL) QSOs in a complete sample of 111 ultravi...
We present the results of European VLBI Network observations of 3 Broad Absorption Line quasars at ...
Context. Broad absorption lines (BALs) are present in the spectra of ~20% of quasars (QSOs); this in...
Multi-frequency 1.7, 5 and 8.4-GHz VLBA observations of a radio-loud broad absorption line (BAL) qua...
Abstract Broad Absorption Lines (BALs) seem to be the most extreme manifestations of quasar (QSO) ou...
We propose a morphological classification based on the parsec scale structure of fifty-one High Freq...