activity
19962023
most citedA distance to the Large Magellanic Cloud that is precise to one per cent

686 citations · 9.6k across the 131 of their papers we have counts for

collaborators
Showing 2014Show all

7 papers · 1 filter

astro-ph.GA2014★ 7 cited

A pilot study using deep infrared imaging to constrain the star formation history of the XUV stellar populations in NGC 4625

Stephanie J. Bush, Robert C. Kennicutt, M. L. N. Ashby +3

In a LCDM universe, disk galaxies' outer regions are the last to form. Characterizing their contents is critical for understanding the ongoing process of disk formation, but observ…

astro-ph.GA2014★ 116 cited

Carbon and oxygen abundances from recombination lines in low-metallicity star-forming galaxies. Implications for chemical evolution

C. Esteban, J. García-Rojas, L. Carigi +4

We present deep echelle spectrophotometry of the brightest emission-line knots of the star-forming galaxies He 2-10, Mkn 1271, NGC 3125, NGC 5408, POX 4, SDSS J1253-0312, Tol 1457-…

astro-ph.GA2014★ 105 cited

The relation for massive bursts of star formation

Ricardo Chávez, Roberto Terlevich, Elena Terlevich +4

The validity of the emission line luminosity vs. ionised gas velocity dispersion () correlation for HII galaxies (HIIGx), and its potential as an accurate distance estimator…

astro-ph.GA2014★ 49 cited

Stellar Metallicity of the Extended Disk and Distance of the Spiral Galaxy NGC 3621

Rolf-Peter Kudritzki, Miguel A. Urbaneja, Fabio Bresolin +2

Low resolution ESO VLT/FORS spectra of blue supergiant stars are analyzed to determine stellar metallicities (based on elements such as Fe, Ti, Mg) in the extended disk of the spir…

astro-ph.GA2014★ 40 cited

A New Method for Measuring Metallicities of Young Super Star Clusters

J. Zachary Gazak, Ben Davies, Nate Bastian +7

We demonstrate how the metallicities of young super star clusters can be measured using novel spectroscopic techniques in the J-band. The near-infrared flux of super star clusters…

astro-ph.GA2014★ 65 cited

Quantitative Spectroscopy of Blue Supergiants in Metal-Poor Dwarf Galaxy NGC 3109

Matthew W. Hosek, Rolf-Peter Kudritzki, Fabio Bresolin +6

We present a quantitative analysis of the low-resolution (4.5 A) spectra of 12 late-B and early-A blue supergiants (BSGs) in the metal-poor dwarf galaxy NGC 3109. A modified method…