RT Journal Article
T1 Spatially resolved analysis of neutralwWinds, stars, and ionized gas kinematics with MEGARA/GTC: new insights on the nearby galaxy UGC 10205
A1 Catalán Torrecilla, C.
A1 Castillo Morales, África
A1 Gil de Paz, Armando
A1 Gallego Maestro, Jesús
A1 Chamorro Cazorla, Mario
A1 Pascual Ramírez, Sergio
A1 Cardiel López, Nicolás
A1 Dullo, Bililign
AB We present a comprehensive analysis of the multiphase structure of the interstellar medium (ISM) and the stellar kinematics in the edge-on nearby galaxy UGC 10205 using integral field spectroscopy (IFS) data taken with MultiEspectrógrafo en GTC de Alta Resolución para Astronomía (MEGARA) at the GTC. We explore both the neutral and the ionized gas phases using the interstellar Na I D doublet absorption (LR−V setup, R ∼ 6000) and the Hα emission line (HR−R setup, R ∼ 18000), respectively. The high-resolution data show the complexity of the Hα emission-line profile revealing the detection of up to three kinematically distinct gaseous components. Despite of this fact, a thin-disk model is able to reproduce the bulk of the ionized gas motions in the central regions of UGC 10205. The use of asymmetric drift corrections is needed to reconciliate the ionized and the stellar velocity rotation curves. We also report the detection of outflowing neutral gas material blueshifted by ∼ 87 km s^(−1) . The main physical properties that describe the observed outflow are a total mass M_(out) = (4.55 ± 0.06) × 10^(7) Mʘ and a coldgas mass outflow rate M_(out) =  0.78   0.03 Mʘ yr^(−1) . This work points out the necessity of exploiting highresolution IFS data to understand the multiphase components of the ISM and the multiple kinematical components in the central regions of nearby galaxies.
PB IOP Publishing Ltd
SN 0004-637X
YR 2020
FD 2020-02-06
LK https://hdl.handle.net/20.500.14352/6196
UL https://hdl.handle.net/20.500.14352/6196
LA eng
NO © 2020. The American Astronomical Society. Artículo firmado por 18 autores. The authors acknowledge financial support from the Spanish Ministry of Economy and Competitiveness (MINECO) under grant No. AYA2016-75808-R, which is partly funded by the European Regional Development Fund (ERDF), AYA2017- 90589-REDT, RTI2018-096188-B-I00, S2018/NMT-4291, and ESP2017-83197P projects. C.C.T. gratefully acknowledges the support of the European Youth Employment Initiative (YEI) by means of the Postdoctoral Fellowship Program. G.B. acknowledges financial support from DGAPAUNAM through PAPIIT project IG100319.
NO Ministerio de Economía y Competitividad (MINECO)/FEDER
NO Comunidad de Madrid
NO DGAPA-UNAM through PAPIIT
NO European Youth Employment Initiative (YEI)
DS Docta Complutense
RD 29 abr 2024