Results 51 to 60 of about 382 (184)
Balmer Absorption in Iron Low-ionization Broad Absorption Line Quasars
While C iv is the most common absorption line in broad absorption line quasar spectra, Balmer absorption lines (BALs) are among the rarest. We present analysis of Balmer absorption in a sample of 14 iron low-ionization BAL quasars (FeLoBALQs); eight are ...
Karen M. Leighly +6 more
doaj +1 more source
Minimalist Footwear Acutely Alters Running Kinematics in Runners With Medial Tibial Stress Syndrome
Purpose To assess immediate biomechanical changes in runners with medial tibial stress syndrome (MTSS) when transitioning from standard to minimalist running shoes. Methods Active runners diagnosed with MTSS ran on a treadmill at 10 km/h using standard and minimalist running shoes. Hip, knee, and ankle joint kinematics were captured using a 16‐infrared‐
Quyet Thang Nguyen +6 more
wiley +1 more source
X-Ray Insights into the Nature of Quasars with Redshifted Broad Absorption Lines [PDF]
Abstract We present Chandra observations of seven broad absorption line (BAL) quasars at with redshifted BAL troughs (RSBALs). Five of our seven targets were detected by Chandra in 4–13 ks exposures with ACIS-S. The
Ning-Xiao Zhang +10 more
openaire +5 more sources
AGN Feedback Efficiency of Narrow Absorption Line Quasars
We consider if outflowing winds that are detected via narrow absorption lines (NALs) with FWHM of
Toru Misawa +2 more
doaj +1 more source
Hidden No More: Spotlight on Tidal Disruption Events in Active Galactic Nuclei
ABSTRACT Tidal disruption events (TDEs) are typically discovered in previously quiescent galaxies. However, earlier studies have revealed a handful of TDEs occurring in pre‐existing active galactic nuclei (AGN). We discuss AT2019aalc, a promising TDE candidate in an AGN, and compare it to similar sources.
Patrik Milán Veres
wiley +1 more source
Low-ionization broad absorption lines in quasars
The absorption line properties of six Mg II broad absorption line quasars (BALQs) are examined using a BALQ sample of Weymann et al. (1991). It is found that Al III absorption is always stronger than Al II absorption; C IV absorption tends to be very deep and broad; and low ionization absorption tends to be narrower and lie at the low velocity end of ...
G. M. Voit +2 more
openaire +1 more source
THE LONG-TERM X-RAY VARIABILITY OF BROAD ABSORPTION LINE QUASARS [PDF]
We analyze the long-term (rest-frame 3-30 yr) X-Ray variability of eleven broad absorption line (BAL) quasars, mainly to constrain the variation properties of the X-Ray absorbing shielding gas that is thought to play a critical role in BAL wind launching. Our BAL quasar sample has coverage with multiple X-ray observatories including Chandra, XMM-Newton,
Saez, C. +4 more
openaire +7 more sources
The Fraction and Kinematics of Broad Absorption Line Quasars across Cosmic Time
Luminous quasars are powerful targets to investigate the role of feedback from supermassive black holes (BHs) in regulating the growth phases of BHs themselves and of their host galaxies, up to the highest redshifts.
Manuela Bischetti +19 more
doaj +1 more source
The anticancer activity of the complexes Pd3Spd2, Pt3Spd2, Pt2Put2(NH3)4 and Pd2Put2 against human TNBC, non‐TNBC and healthy breast cells was evaluated. The metabolic impact of the most promising metal complexes—Pd3Spd2 and Pt2Put2(NH3)4—was further assessed using vibrational microspectroscopies, providing detailed insights into the drug‐induced ...
Clara B. Martins +3 more
wiley +1 more source
The Frequency and Radio Properties of Broad Absorption Line Quasars [PDF]
A sample of 67 Broad Absorption Line quasars (BALQSOs) from the Large Bright Quasar Survey (LBQS) is used to estimate the observed and intrinsic fraction of BAL quasars in optically--selected samples at intermediate (B_J \simeq 18.5) magnitudes. The observed BALQSO fraction in the redshift range 1.5 < z < 3.0 is 15\pm3%.
Hewett, Paul C., Foltz, Craig B.
openaire +2 more sources

