TY  - JOUR
TI  - LeMMINGs - II. The e-MERLIN legacy survey of nearby galaxies. The deepest radio view of the Palomar sample on parsec scale
AV  - public
Y1  - 2021/02/01/
EP  - 4767
N2  - We present the second data release of high-resolution (?0.2 arcsec) 1.5-GHz radio images of 177 nearby galaxies from the Palomar sample, observed with the e-MERLIN array, as part of the Legacy e-MERLIN Multi-band Imaging of Nearby Galaxies Sample (LeMMINGs) survey. Together with the 103 targets of the first LeMMINGs data release, this represents a complete sample of 280 local active (LINER and Seyfert) and inactive galaxies (H?II galaxies and absorption line galaxies, ALG). This large program is the deepest radio survey of the local Universe, ?1017.6 W Hz?1, regardless of the host and nuclear type: we detect radio emission ?0.25 mJy beam?1 for 125/280 galaxies (44.6 per?cent) with sizes of typically ?100 pc. Of those 125, 106 targets show a core which coincides within 1.2 arcsec with the optical nucleus. Although we observed mostly cores, around one third of the detected galaxies features jetted morphologies. The detected radio core luminosities of the sample range between ?1034 and 1040 erg s?1. LINERs and Seyferts are the most luminous sources, whereas H?II galaxies are the least. LINERs show FR I-like core-brightened radio structures while Seyferts reveal the highest fraction of symmetric morphologies. The majority of H?II galaxies have single radio core or complex extended structures, which probably conceal a nuclear starburst and/or a weak active nucleus (seven of them show clear jets). ALGs, which are typically found in evolved ellipticals, although the least numerous, exhibit on average the most luminous radio structures, similar to LINERs.
ID  - discovery10121437
PB  - OXFORD UNIV PRESS
KW  - Science & Technology
KW  -  Physical Sciences
KW  -  Astronomy & Astrophysics
KW  -  galaxies: active
KW  -  galaxies: jet
KW  -  galaxies: nuclei
KW  -  galaxies: star formation
KW  -  radio continuum: galaxies
KW  -  ACTIVE GALACTIC NUCLEI
KW  -  SUPERMASSIVE BLACK-HOLES
KW  -  INDUCED STAR-FORMATION
KW  -  DWARF SEYFERT NUCLEI
KW  -  SUPERNOVA-REMNANTS
KW  -  X-RAY
KW  -  LUMINOSITY FUNCTION
KW  -  LIMITED SAMPLE
KW  -  EMISSION
KW  -  ORIGIN
SP  - 4749
VL  - 500
IS  - 4
N1  - This version is the version of record. For information on re-use, please refer to the publisher?s terms and conditions.
UR  - https://doi.org/10.1093/mnras/staa3519
JF  - Monthly Notices of the Royal Astronomical Society
A1  - Baldi, RD
A1  - Williams, DRA
A1  - McHardy, IM
A1  - Beswick, RJ
A1  - Brinks, E
A1  - Dullo, BT
A1  - Knapen, JH
A1  - Argo, MK
A1  - Aalto, S
A1  - Alberdi, A
A1  - Baan, WA
A1  - Bendo, GJ
A1  - Corbel, S
A1  - Fenech, DM
A1  - Gallagher, JS
A1  - Green, DA
A1  - Kennicutt, RC
A1  - Kloeckner, H-R
A1  - Koerding, E
A1  - Maccarone, TJ
A1  - Muxlow, TWB
A1  - Mundell, CG
A1  - Panessa, F
A1  - Peck, AB
A1  - Perez-Torres, MA
A1  - Romero-Canizales, C
A1  - Saikia, P
A1  - Shankar, F
A1  - Spencer, RE
A1  - Stevens, IR
A1  - Varenius, E
A1  - Ward, MJ
A1  - Yates, J
A1  - Uttley, P
ER  -