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19992026
most citedSupermassive black hole formation during the assembly of pre-galactic discs

490 citations · 839 across the 26 of their papers we have counts for

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astro-ph2008★ 66 cited

Pre-peak ram pressure stripping in the Virgo cluster spiral galaxy NGC 4501

B. Vollmer, M. Soida, A. Chung +5

VIVA HI observations of the Virgo spiral galaxy NGC 4501 are presented. The HI disk is sharply truncated to the southwest, well within the stellar disk. A region of low surface-den…

astro-ph2006★ 490 cited

Supermassive black hole formation during the assembly of pre-galactic discs

Giuseppe Lodato, Priya Natarajan

In this paper we discuss the evolution of gravitationally unstable pre-galactic discs that result from the collapse of haloes at high redshift or so, which have not…

astro-ph2005★ 26 cited

Core Overshoot: An Improved Treatment and Constraints from Seismic Data

Christian W. Straka, Pierre Demarque, D. B. Guenther

We present a comprehensive set of stellar evolution models for Procyon A in an effort to guide future measurements of both traditional stellar parameters and seismic frequencies to…

astro-ph2005★ 16 cited

The CIDA-UCM-Yale Shallow Survey for Emission Line Galaxies

A. Bongiovanni, G. Bruzual, G. Magris +4

We present the CIDA-UCM-Yale (Centro de Investigaciones de Astronomia, Universidad Complutense de Madrid and Yale University) survey for Halpha+[NII]6549,6584 emission-line galaxie…

astro-ph2004

Searching for White and Brown Dwarfs in the frame of the MUSYC/CYDER survey

M. Altmann, R. A. M'endez, M. -T. Ruiz +4

MUSYC (MUltiwavelength Survey by Yale and Chile), and its predecessor, the CYDER (Cal'an Yale Deep Extragalactic Research) survey are both deep multiwavelength surveys mainly aimin…

astro-ph2004★ 99 cited

Radio continuum observations of the Virgo cluster spiral NGC 4522 The signature of ram pressure

B. Vollmer, R. Beck, J. D. P. Kenney +1

Radio continuum observations at 20 and 6 cm of the highly inclined Virgo spiral galaxy NGC 4522 are presented. Both, 20 and 6 cm total emission distributions are asymmetric with an…