The Origin of Faint Tidal Features around Galaxies in the RESOLVE Survey
Abstract
We study tidal features around galaxies in the REsolved Spectroscopy Of a Local VolumE (RESOLVE) survey. Our sample consists of 1048 RESOLVE galaxies that overlap with the DECam Legacy Survey, which reaches an $$r$$-band 3$$σ$$ depth of ~27.9 mag arcsec-2 for a 100 arcsec2 feature. Images were masked, smoothed, and inspected for tidal features such as streams, shells, or tails/arms. We find tidal features in 17±2% of our galaxies, setting a lower limit on the true frequency. The frequency of tidal features in the gas-poor (gas-to-stellar mass ratio <0.1) subsample is lower than in the gas-rich subsample (13±3% versus 19±2%). Within the gas-poor subsample, galaxies with tidal features have higher stellar and halo masses, ~3× closer distances to nearest neighbors (in the same group), and possibly fewer group members at fixed halo mass than galaxies without tidal features, but similar specific star formation rates. These results suggest tidal features in gas-poor galaxies are typically streams/shells from dry mergers or satellite disruption. In contrast, the presence of tidal features around gas-rich galaxies does not correlate with stellar or halo mass, suggesting these tidal features are often tails/arms from resonant interactions. Similar to tidal features in gas-poor galaxies, tidal features in gas-rich galaxies imply 1.7× closer nearest neighbors in the same group; however, they are associated with diskier morphologies, higher star formation rates, and higher gas content. In addition to interactions with known neighbors, we suggest that tidal features in gas-rich galaxies may arise from accretion of cosmic gas and/or gas-rich satellites below the survey limit.
- Authors:
-
[1];
[2];
[1];
- Univ. of North Carolina, Chapel Hill, NC (United States). Dept. of Physics and Astronomy
- Univ. of North Carolina, Chapel Hill, NC (United States). Dept. of Physics and Astronomy; Univ. of Tokyo (Japan)
- Brown Univ., Providence, RI (United States). Dept. of Physics
- Univ. of Central Lancashire, Lancashire (England)
- Columbia Univ., New York, NY (United States). Dept. of Physics
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1544057
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 857; Journal Issue: 2; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics
Citation Formats
Hood, Callie E., Kannappan, Sheila J., Stark, David V., Dell’Antonio, Ian P., Moffett, Amanda J., Eckert, Kathleen D., Norris, Mark A., and Hendel, David. The Origin of Faint Tidal Features around Galaxies in the RESOLVE Survey. United States: N. p., 2018.
Web. doi:10.3847/1538-4357/aab719.
Hood, Callie E., Kannappan, Sheila J., Stark, David V., Dell’Antonio, Ian P., Moffett, Amanda J., Eckert, Kathleen D., Norris, Mark A., & Hendel, David. The Origin of Faint Tidal Features around Galaxies in the RESOLVE Survey. United States. https://doi.org/10.3847/1538-4357/aab719
Hood, Callie E., Kannappan, Sheila J., Stark, David V., Dell’Antonio, Ian P., Moffett, Amanda J., Eckert, Kathleen D., Norris, Mark A., and Hendel, David. Fri .
"The Origin of Faint Tidal Features around Galaxies in the RESOLVE Survey". United States. https://doi.org/10.3847/1538-4357/aab719. https://www.osti.gov/servlets/purl/1544057.
@article{osti_1544057,
title = {The Origin of Faint Tidal Features around Galaxies in the RESOLVE Survey},
author = {Hood, Callie E. and Kannappan, Sheila J. and Stark, David V. and Dell’Antonio, Ian P. and Moffett, Amanda J. and Eckert, Kathleen D. and Norris, Mark A. and Hendel, David},
abstractNote = {We study tidal features around galaxies in the REsolved Spectroscopy Of a Local VolumE (RESOLVE) survey. Our sample consists of 1048 RESOLVE galaxies that overlap with the DECam Legacy Survey, which reaches an $r$-band 3$σ$ depth of ~27.9 mag arcsec-2 for a 100 arcsec2 feature. Images were masked, smoothed, and inspected for tidal features such as streams, shells, or tails/arms. We find tidal features in 17±2% of our galaxies, setting a lower limit on the true frequency. The frequency of tidal features in the gas-poor (gas-to-stellar mass ratio <0.1) subsample is lower than in the gas-rich subsample (13±3% versus 19±2%). Within the gas-poor subsample, galaxies with tidal features have higher stellar and halo masses, ~3× closer distances to nearest neighbors (in the same group), and possibly fewer group members at fixed halo mass than galaxies without tidal features, but similar specific star formation rates. These results suggest tidal features in gas-poor galaxies are typically streams/shells from dry mergers or satellite disruption. In contrast, the presence of tidal features around gas-rich galaxies does not correlate with stellar or halo mass, suggesting these tidal features are often tails/arms from resonant interactions. Similar to tidal features in gas-poor galaxies, tidal features in gas-rich galaxies imply 1.7× closer nearest neighbors in the same group; however, they are associated with diskier morphologies, higher star formation rates, and higher gas content. In addition to interactions with known neighbors, we suggest that tidal features in gas-rich galaxies may arise from accretion of cosmic gas and/or gas-rich satellites below the survey limit.},
doi = {10.3847/1538-4357/aab719},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 857,
place = {United States},
year = {Fri Apr 20 00:00:00 EDT 2018},
month = {Fri Apr 20 00:00:00 EDT 2018}
}
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Figure 1: A comparison of the SDSS (left), DECaLS (middle), and IAC (right) images of the galaxy rf0358. The deeper DECaLS and IAC images reveal the faint extension on the left side of the galaxy.
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Post-merger Signatures of Red-sequence Galaxies in Rich Abell Clusters at $z\lesssim 0.1$
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Faint Tidal Features in Galaxies within the Canada-France-Hawaii Telescope Legacy Survey Wide Fields
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How well does the Friends-of-Friends algorithm recover group properties from galaxy catalogs limited in both distance and luminosity?
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The neutral gas content of post-merger galaxies
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RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
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Surface density effects in quenching: cause or effect?
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Quantifying the impact of mergers on the angular momentum of simulated galaxies
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Linking Gas Fractions to Bimodalities in Galaxy Properties
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Lopsided spiral galaxies: evidence for gas accretion
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Percolation Galaxy Groups and Clusters in the SDSS Redshift Survey: Identification, Catalogs, and the Multiplicity Function
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Formation of S0 galaxies through mergers: Morphological properties: tidal relics, lenses, ovals, and other inner components⋆
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Identification of Low Surface Brightness Tidal Features in Galaxies Using Convolutional Neural Networks
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The Halos and Environments of Nearby Galaxies (HERON) I: Imaging, Sample Characteristics, and Envelope Diameters
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