output
19942026
most citedThe Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

2.5k citations

Showing 2004 · astro-phShow all

8 papers · 2 filters

astro-ph2004★ 16 cited

The age of the Galactic thin disk from Th/Eu nucleocosmochronology II. Chronological analysis

E. F. del Peloso, L. da Silva, L. I. Arany-Prado

The purpose of this work is to resume investigation of Galactic thin disk dating using nucleocosmochronology with Th/Eu stellar abundance ratios, a theme absent from the literature…

astro-ph2004★ 26 cited

The age of the Galactic thin disk from Th/Eu nucleocosmochronology I. Determination of [Th/Eu] abundance ratios

E. F. del Peloso, L. da Silva, G. F. Porto de Mello

The purpose of this work is to resume investigation of Galactic thin disk dating using nucleocosmochronology with Th/Eu stellar abundance ratios, a theme absent from the literature…

astro-ph2004★ 42 cited

Fine structure of the chromospheric activity in Solar-type stars - The Halpha Line

W. Lyra, G. F. Porto de Mello

A calibration of H-alpha as both a chromospheric diagnostic and an age indicator is presented, complementing the works previously done on this subject (Herbig 1985, Pasquini & Pall…

astro-ph2004★ 6 cited

The Aquarius Superclusters II. Spectroscopic and Photometric Data

Cesar A. Caretta, Marcio A. G. Maia, Christopher N. A. Willmer

We present spectroscopic and photometric data for 920 galaxies selected in 68 fields of the Aquarius Cluster Catalog. Typically the 15 brightest candidate members with magnitudes i…

astro-ph2004

The outflowing disks of B[e] supergiants and unclassified B[e] stars

Michaela Kraus, Marcelo Borges Fernandes

B[e] supergiants are known to possess outflowing cool disks but also some unclassified B[e] stars show clear indications for the presence of a neutral disk. We derive constraints o…

astro-ph2004★ 134 cited

Sub-Galactic Clumps at High Redshift: A Fragmentation Origin?

Andreas Immeli, Markus Samland, Pieter Westera +1

We investigate the origin of the clumpy structures observed at high redshift, like the chain galaxies. We use a three dimensional chemodynamical simulation describing the dynamics…