TY - JOUR
T1 - A Large Jet Narrow-line Seyfert 1 Galaxy
T2 - Observations from Parsec to 100 kpc Scales
AU - Chen, Sina
AU - Kharb, Preeti
AU - Sasikumar, Silpa
AU - Nandi, Sumana
AU - Berton, Marco
AU - Järvelä, Emilia
AU - Laor, Ari
AU - Behar, Ehud
AU - Foschini, Luigi
AU - Vietri, Amelia
AU - Gu, Minfeng
AU - La Mura, Giovanni
AU - Crepaldi, Luca
AU - Zhou, Minhua
N1 - Publisher Copyright:
© 2024 Institute of Physics. All rights reserved.
PY - 2024/3/1
Y1 - 2024/3/1
N2 - We present new 1.5-8.5 GHz Very Long Baseline Array (VLBA) observations and 0.32-1.26 GHz Giant Meterwave Radio Telescope (GMRT) observations of J0354-1340, which is the only known radio-quiet (RQ) or radio-intermediate (RI) narrow-line Seyfert 1 galaxy with a 100 kpc, two-sided radio jet. A parsec-scale, one-sided jet in the southeastern direction from the core emission is found in the VLBA observations, while the kiloparsecscale jet observed with the Karl G. Jansky Very Large Array (VLA) and GMRT is in the south-north direction. Core spectra on parsec and kiloparsec scales are presented in combination with archival VLA Sky Survey observations at 3.0 GHz and VLA C-configuration observations at 5.5 GHz. The parsec-scale emission dominates the kiloparsec-scale emission above ~5 GHz, and the spectrum is inverted due to synchrotron self-absorption. This indicates a compact synchrotron source with a size of ~0.04 pc, which is associated with either the jet base or the corona. A subkiloparsec-scale jet, which is unresolved on scales of ~3", probably dominates the emission below ~5 GHz. Future radio observations can explore the jet structure between the parsec and 100 kpc scales, the origin of their direction mismatch, and the parsec-scale jet proper motion. It remains to be explored how common such large-scale jets are in RQ or RI active galactic nuclei.
AB - We present new 1.5-8.5 GHz Very Long Baseline Array (VLBA) observations and 0.32-1.26 GHz Giant Meterwave Radio Telescope (GMRT) observations of J0354-1340, which is the only known radio-quiet (RQ) or radio-intermediate (RI) narrow-line Seyfert 1 galaxy with a 100 kpc, two-sided radio jet. A parsec-scale, one-sided jet in the southeastern direction from the core emission is found in the VLBA observations, while the kiloparsecscale jet observed with the Karl G. Jansky Very Large Array (VLA) and GMRT is in the south-north direction. Core spectra on parsec and kiloparsec scales are presented in combination with archival VLA Sky Survey observations at 3.0 GHz and VLA C-configuration observations at 5.5 GHz. The parsec-scale emission dominates the kiloparsec-scale emission above ~5 GHz, and the spectrum is inverted due to synchrotron self-absorption. This indicates a compact synchrotron source with a size of ~0.04 pc, which is associated with either the jet base or the corona. A subkiloparsec-scale jet, which is unresolved on scales of ~3", probably dominates the emission below ~5 GHz. Future radio observations can explore the jet structure between the parsec and 100 kpc scales, the origin of their direction mismatch, and the parsec-scale jet proper motion. It remains to be explored how common such large-scale jets are in RQ or RI active galactic nuclei.
UR - http://www.scopus.com/inward/record.url?scp=85188215017&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ad182a
DO - 10.3847/1538-4357/ad182a
M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???
AN - SCOPUS:85188215017
SN - 0004-637X
VL - 963
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1
M1 - 32
ER -