Optical spectroscopy of nearby type1-LINERs


Por: Cazzoli S., Márquez I., Masegosa J., Del Olmo A., Povic M., González-Martín O., Balmaverde B., Hernández-García L., García-Burillo S.

Ahead of Print: 1 ene 2021
Resumen:
We present the highlights from our recent study of 22 local (z < 0.025) type-1 LINERs from the Palomar Survey, on the basis of optical long-slit spectroscopic observations taken with TWIN/CAHA, ALFOSC/NOT and HST/STIS. Our goals were threefold: (a) explore the AGN-nature of these LINERs by studying the broad (BLR-originated) Ha? 6563 component; (b) derive a reliable interpretation for the multiple narrow components of emission lines by studying their kinematics and ionisation mechanism (via standard BPTs); (c) probe the neutral gas in the nuclei of these LINERs for the first time. Hence, kinematics and fluxes of a set of emission lines, from Hß ?4861 to [SII]?? 716,6731, and the NaD??5890,5896 doublet in absorption have been modelled and measured, after the subtraction of the underlying light from the stellar component. © The Author(s), 2021.

Filiaciones:
Cazzoli S.:
 IAA - Instituto de Astrofísica de Andalucía (CSIC), Apdo. 3004, Granada, 18080, Spain

Márquez I.:
 IAA - Instituto de Astrofísica de Andalucía (CSIC), Apdo. 3004, Granada, 18080, Spain

Masegosa J.:
 IAA - Instituto de Astrofísica de Andalucía (CSIC), Apdo. 3004, Granada, 18080, Spain

Del Olmo A.:
 IAA - Instituto de Astrofísica de Andalucía (CSIC), Apdo. 3004, Granada, 18080, Spain

Povic M.:
 IAA - Instituto de Astrofísica de Andalucía (CSIC), Apdo. 3004, Granada, 18080, Spain

 ESSTI/EORC, Ethiopian Space Science and Technology Institute, Entoto Observatory and Research Center, P.O. Box 33679, Addis Ababa, Ethiopia

González-Martín O.:
 IRyA - Instituto de Radioastronomía y Astrofísica, 3-72 Xangari, Morelia, 8701, Mexico

Balmaverde B.:
 INAF, Osservatorio Astronomico di Brera, via Brera 28, Milano, I-20121, Italy

Hernández-García L.:
 Universidad de Valparaíso, Gran Bretana 1111, Playa Ancha, Valparaíso, Chile

García-Burillo S.:
 OAN, Observatorio Astronómico Nacional, Alfonso XII, 3, Madrid, 28014, Spain
ISSN: 17439213
Editorial
CAMBRIDGE UNIV PRESS, THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND, Reino Unido
Tipo de documento: Conference Paper
Volumen: Número:
Páginas: 87-92
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