Results 1 to 10 of about 910,975 (204)

B2 1144+35B, a giant low power radio galaxy with superluminal motion. Orientation and evidence for recurrent activity [PDF]

, 2007
The goal of this work is a detailed study of the nearby, low power radio galaxy B2 1144+35B. For this purpose, we performed new Very Long Baseline Array (VLBA) and Very Large Array (VLA) observations.
Allen, Colla, Croft, Ekers, G. B. Taylor, G. Giovannini, Giovannini, Giovannini, Giovannini, Giovannini, Giroletti, M. Giroletti, Machalski, Marcha, Mirabel, Morganti, Taylor   +16 more
core   +1 more source

SDSS J124602.54+011318.8: A Highly Variable AGN, Not an Orphan GRB Afterglow [PDF]

, 2002
The optically variable source SDSS J124602.54+011318.8 first appears in Sloan Digital Sky Survey (SDSS) data as a bright point source with nonstellar colors.
Alexei V. Filippenko, Avishay Gal‐Yam, Browne I. W. A., Eran O. Ofek, Kock A., Marcha M. J. M., Marcha M. J. M., Nass P., Rest A., Ryan Chornock, Stickel M., Weidong Li   +11 more
core   +2 more sources

Las fuerzas con efecto transiente durante la marcha militar [PDF]

, 2013
Introdução: O padrão vertical anormal da força de reação do solo (FRS) apresenta a assimetria ou mais de dois picos como marcha patológica típica. Uma força típica e assimétrica é a força transiente.
Amadio, Alberto Carlos, Guisande, Thais Pereira, Mochizuki, Luis, Serrão, Julio Cerca   +3 more
core   +2 more sources

Blazar Counterparts for 3EG Sources at -40 < decl. < 0: Pushing South Through the Bulge [PDF]

, 2004
Supplementing existing survey data with VLA observations, we have extended $\gamma-$ray counterpart identifications down to decl. = -40$^\circ$ using our Figure of Merit approach. We find blazar counterparts for $\sim$ 70% of EGRET sources above decl. = -
David Sowards‐Emmerd, James S. Ulvestad, Marcha M. J. M., Peter F. Michelson, Roger W. Romani   +4 more
core   +1 more source

Momento aductor de la cadera durante la marcha en adultos mayores asintomáticos

Universidad y Salud, 2021
Introducción: El momento articular durante la marcha se ha relacionado con diferentes procesos clínicos en la población adulto mayor, en Colombia no se cuentan con reportes propios.
José David Vélez-Uribe, Ana María Mejía-Uñates, Sara Teresa Piedrahita-Roldán, Tatiana Ramírez-Estrada, Nicolás Eugenio Gómez-Suárez, José Ricardo Duque-Ramírez   +5 more
doaj   +1 more source

WISE colours and star-formation in the host galaxies of radio-loud narrow-line Seyfert 1 [PDF]

, 2015
We investigate the mid-infrared properties of the largest (42 objects) sample of radio-loud narrow-line Seyfert 1 (RL NLS1) collected to date, using data from the Wide-field Infrared Survey Explorer (WISE).
Anton, S., Ballo, L., Caccianiga, A., Della Ceca, R., Foschini, L., Maccacaro, T., Marcha, M. J., Mateos, S., Sani, E., Severgnini, P.   +9 more
core   +2 more sources

The effect of Kathak Dance Movement on Balance and Gait in Parkinson’s Disease- An Experimental Study

Revista Pesquisa em Fisioterapia, 2022
INTRODUCTION: Difficulties with gait and balance are common among individuals with Parkinson's disease (PD). Several different exercise programs have been suggested to address balance and gait problems to improve the quality of life and patient ...
Deepika Metange, Loveleen Waghule, Medha Deo   +2 more
doaj   +1 more source

Justicia transicional

Análisis Jurídico - Político
Existe la necesidad de comprender a profundidad cómo los factores humanos influyen en la efectividad de la justicia, junto a los esfuerzos por implementar medidas de reparación y reconciliación.
Jorge Andrés Arboleda Montalvo, Adrián Esteban Cardozo Duque   +1 more
doaj   +1 more source

The CLASS BL Lac sample: The Radio Luminosity Function

, 2013
This paper presents a new sample of BL Lac objects selected from a deep (30 mJy) radio survey of flat spectrum radio sources (the CLASS blazar survey, henceforth CBS).
Caccianiga, A., Marcha, M. J. M.
core   +1 more source

The colour of the narrow line Sy1-blazar 0324+3410

, 2008
Aims. We investigate the properties of the host galaxy of the blazar J0324+3410 (B2 0321+33) by the analysis of B and R images obtained with the NOT under good photometric conditions.
Anton, S., Browne, I. W. A., Marcha, M. J.   +2 more
core   +2 more sources