Abstract / Description of output
We present new Spectrographic Areal Unit for Research on Optical Nebulae
(SAURON) integral-field spectroscopy and Swift Ultraviolet Optical
Telescope (UVOT) observations of molecular outflow host galaxy NGC 1266
that indicate NGC 1266 has experienced a rapid cessation of star
formation. Both the SAURON maps of stellar population age and the Swift
UVOT observations demonstrate the presence of young (~ 1 Gyr by cyclically injecting turbulent energy into the
dense molecular gas via a radio jet, inhibiting star formation.
Original language | English |
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Pages (from-to) | 186 |
Journal | Astrophysical Journal |
Volume | 780 |
Issue number | 2 |
DOIs | |
Publication status | Published - 1 Jan 2014 |
Keywords / Materials (for Non-textual outputs)
- galaxies: active
- galaxies: evolution
- galaxies: individual: NGC 1266