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Title: HST/ACS DIRECT AGES OF THE DWARF ELLIPTICAL GALAXIES NGC 147 AND NGC 185

Abstract

We present the deepest optical photometry for any dwarf elliptical (dE) galaxy based on Hubble Space Telescope Advanced Camera for Surveys (ACS) observations of the Local Group dE galaxies NGC 147 and NGC 185. Our F606W and F814W color–magnitude diagrams are the first to reach below the oldest main sequence turnoff in a dE galaxy, allowing us to determine full star formation histories in these systems. The ACS fields are located roughly ∼1.5 effective radii from the galaxy center to avoid photometric crowding. While both ACS fields show unambiguous evidence for old and intermediate age stars, the mean age of NGC 147 is ∼4–5 Gyr younger as compared to NGC 185. In NGC 147, only 40% of stars were in place 12.5 Gyr ago (z ∼ 5), with the bulk of the remaining stellar population forming between 5 to 7 Gyr. In contrast, 70% of stars were formed in NGC 185 prior to 12.5 Gyr ago with the majority of the remaining population forming between 8 to 10 Gyr ago. Star formation has ceased in both ACS fields for at least 3 Gyr. Previous observations in the central regions of NGC 185 show evidence for star formation as recent asmore » 100 Myr ago, and a strong metallicity gradient with radius. This implies a lack of radial mixing between the center of NGC 185 and our ACS field. The lack of radial gradients in NGC 147 suggests that our inferred SFHs are more representative of its global history. We interpret the inferred differences in star formation histories to imply an earlier infall time into the M31 environment for NGC 185 as compared to NGC 147.« less

Authors:
 [1];  [2];  [3];  [4];  [5];  [6]
  1. Astronomy Department, Yale University, New Haven, CT 06520 (United States)
  2. Astronomy Department, Box 351580, University of Washington, Seattle, WA 98195 (United States)
  3. Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803 (United States)
  4. Raytheon, 1151 E. Hermans Road, Tucson, AZ 85756 (United States)
  5. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States)
  6. UCO/Lick Observatory, University of California, Santa Cruz, 1156 High Street, Santa Cruz, CA 95064 (United States)
Publication Date:
OSTI Identifier:
22525332
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal; Journal Volume: 811; Journal Issue: 2; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; CAMERAS; COLOR; DIAGRAMS; GALAXIES; GALAXY CLUSTERS; METALLICITY; PHOTOMETRY; SPACE; STAR CLUSTERS; STAR EVOLUTION; STARS; TELESCOPES

Citation Formats

Geha, M., Weisz, D., Grocholski, A., Dolphin, A., Marel, R. P. van der, and Guhathakurta, P., E-mail: marla.geha@yale.edu. HST/ACS DIRECT AGES OF THE DWARF ELLIPTICAL GALAXIES NGC 147 AND NGC 185. United States: N. p., 2015. Web. doi:10.1088/0004-637X/811/2/114.
Geha, M., Weisz, D., Grocholski, A., Dolphin, A., Marel, R. P. van der, & Guhathakurta, P., E-mail: marla.geha@yale.edu. HST/ACS DIRECT AGES OF THE DWARF ELLIPTICAL GALAXIES NGC 147 AND NGC 185. United States. doi:10.1088/0004-637X/811/2/114.
Geha, M., Weisz, D., Grocholski, A., Dolphin, A., Marel, R. P. van der, and Guhathakurta, P., E-mail: marla.geha@yale.edu. 2015. "HST/ACS DIRECT AGES OF THE DWARF ELLIPTICAL GALAXIES NGC 147 AND NGC 185". United States. doi:10.1088/0004-637X/811/2/114.
@article{osti_22525332,
title = {HST/ACS DIRECT AGES OF THE DWARF ELLIPTICAL GALAXIES NGC 147 AND NGC 185},
author = {Geha, M. and Weisz, D. and Grocholski, A. and Dolphin, A. and Marel, R. P. van der and Guhathakurta, P., E-mail: marla.geha@yale.edu},
abstractNote = {We present the deepest optical photometry for any dwarf elliptical (dE) galaxy based on Hubble Space Telescope Advanced Camera for Surveys (ACS) observations of the Local Group dE galaxies NGC 147 and NGC 185. Our F606W and F814W color–magnitude diagrams are the first to reach below the oldest main sequence turnoff in a dE galaxy, allowing us to determine full star formation histories in these systems. The ACS fields are located roughly ∼1.5 effective radii from the galaxy center to avoid photometric crowding. While both ACS fields show unambiguous evidence for old and intermediate age stars, the mean age of NGC 147 is ∼4–5 Gyr younger as compared to NGC 185. In NGC 147, only 40% of stars were in place 12.5 Gyr ago (z ∼ 5), with the bulk of the remaining stellar population forming between 5 to 7 Gyr. In contrast, 70% of stars were formed in NGC 185 prior to 12.5 Gyr ago with the majority of the remaining population forming between 8 to 10 Gyr ago. Star formation has ceased in both ACS fields for at least 3 Gyr. Previous observations in the central regions of NGC 185 show evidence for star formation as recent as 100 Myr ago, and a strong metallicity gradient with radius. This implies a lack of radial mixing between the center of NGC 185 and our ACS field. The lack of radial gradients in NGC 147 suggests that our inferred SFHs are more representative of its global history. We interpret the inferred differences in star formation histories to imply an earlier infall time into the M31 environment for NGC 185 as compared to NGC 147.},
doi = {10.1088/0004-637X/811/2/114},
journal = {Astrophysical Journal},
number = 2,
volume = 811,
place = {United States},
year = 2015,
month =
}
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