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19982022
most citedStar formation sustained by gas accretion

213 citations · 1.6k across the 53 of their papers we have counts for

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8 papers · 1 filter

astro-ph.CO2013★ 70 cited

Local tadpole galaxies: dynamics and metallicity

J. Sanchez Almeida, C. Munoz-Tunon, D. M. Elmegreen +2

Tadpole galaxies, with a bright peripheral clump on a faint tail, are morphological types unusual in the nearby universe but very common early on. Low mass local tadpoles were iden…

astro-ph.CO2012★ 139 cited

SHARDS: an optical spectro-photometric survey of distant galaxies

Pablo G. Perez-Gonzalez, Antonio Cava, Guillermo Barro +26

(Abridged) We present the Survey for High-z Absorption Red and Dead Sources (SHARDS), an ESO/GTC Large Program carried out with GTC/OSIRIS. SHARDS is an ultra-deep optical spectro-…

astro-ph.CO2012★ 46 cited

Local Tadpole Galaxies

Debra Meloy Elmegreen, Bruce G. Elmegreen, Jorge Sanchez Almeida +3

Tadpole galaxies have a giant star-forming region at the end of an elongated intensity distribution. Here we use SDSS data to determine the ages, masses, and surface densities of t…

astro-ph.CO2011★ 19 cited

Relationship between Hubble type and spectroscopic class in local galaxies

J. Sanchez Almeida, J. A. L. Aguerri, C. Munoz-Tunon +1

We compare the Hubble type and the spectroscopic class of the galaxies with spectra in SDSS/DR7. As it is long known, elliptical galaxies tend to be red whereas spiral galaxies ten…

astro-ph.CO2011

Ionization Conditions in the Central Giant HII Region of NGC 5253

A. Monreal-Ibero, J. M. Vílchez, J. Walsh +1

We are carrying out a detailed 2D spectroscopic study of the central 210 pc X 130 pc of the blue compact dwarf (BCD) galaxy NGC5253. This contribution presents the ionization condi…

astro-ph.CO2009★ 18 cited

On the Heating Efficiency Derived from Observations of Young Super Star Clusters in M82

Sergiy Silich, Guillermo Tenorio-Tagle, Ana Torres Campos +2

Here we discuss the mechanical feedback that massive stellar clusters provide to the interstellar medium of their host galaxy. We apply an analytic theory developed in a previous s…