A Near- and Mid-Infrared Study of the Interacting Galaxy Pair UGC 12914/12915: “Taffy”
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1538-3881/118/i=5/a=2132/pdf
Reference42 articles.
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3. Dynamics of Interacting Galaxies
4. Boulanger, F. 1998, in IAU Symp. 179, New Horizons from Multi-Wavelength Sky Surveys, ed. B. J. McLean, D. A. Golombek, J. J. E. Hayes, & H. E. Payne (Dordrecht: Kluwer), 153
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1. The CO Emission in the Taffy Galaxies (UGC 12914/15) at 60 pc Resolution. I. The Battle for Star Formation in the Turbulent Taffy Bridge;The Astrophysical Journal;2022-06-01
2. H i study of isolated and paired galaxies: the MIR SFR-M⋆ sequence;Monthly Notices of the Royal Astronomical Society;2020-10-05
3. Evidence for Shock-heated Gas in the Taffy Galaxies and Bridge from Optical Emission-line IFU Spectroscopy;The Astrophysical Journal;2019-06-25
4. HerschelSpectroscopy of the Taffy Galaxies (UGC 12914/12915 = VV 254): Enhanced [C ii] Emission in the Collisionally Formed Bridge;The Astrophysical Journal;2018-03-16
5. X-RAY EMISSION FROM THE TAFFY (VV254) GALAXIES AND BRIDGE;The Astrophysical Journal;2015-10-14
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