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20022009
most citedThe ACS Nearby Galaxy Survey Treasury

564 citations

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12 papers · 1 filter

astro-ph200724 cited

New Probable Dwarf Galaxies in Northern Groups of the Local Supercluster

I. D. Karachentsev, V. E. Karachentseva, W. K. Huchtmeier

We have searched for nearby dwarf galaxies in 27 northern groups with characteristic distances 8-15 Mpc based on the Second Palomar Sky Survey prints. In a total area of about 2000…

astro-ph2007212 cited

The primordial abundance of 4He: a self-consistent empirical analysis of systematic effects in a large sample of low-metallicity HII regions

Y. I. Izotov, T. X. Thuan, G. Stasinska

We determine the primordial helium mass fraction Yp using 93 spectra of 86 low-metallicity extragalactic HII regions. This sample constitutes the largest and most homogeneous high-…

astro-ph200778 cited

On the maximum value of the cosmic abundance of oxygen and the oxygen yield

L. S. Pilyugin, T. X. Thuan, J. M. Vilchez

We search for the maximum oxygen abundance in spiral galaxies. Because this maximum value is expected to occur in the centers of the most luminous galaxies, we have constructed the…

astro-ph200635 cited

Experimental Ti I oscillator strengths and their application to cool star analysis

R. J. Blackwell-Whitehead, H. Lundberg, G. Nave +5

We report experimental oscillator strengths for 88 Ti I transitions covering the wavelength range 465 to 3892 nm, 67 of which had no previous experimental values. Radiative lifetim…

astro-ph200630 cited

On the electron temperature determination in high-metallicity HII regions

L. S. Pilyugin

The problem of determination of the electron temperature t_2 in the OII zone of high-metallicity HII region was examined. It was shown that the ratio of nebular to auroral nitrogen…

astro-ph200616 cited

The Spitzer View of Low-Metallicity Star Formation: I. Haro 3

L. K. Hunt, T. X. Thuan, M. Sauvage +1

We present Spitzer observations of the blue compact dwarf galaxy (BCD) Haro 3, with an oxygen abundance of 12+log(O/H)=8.32. These data are part of a larger study of star formation…