CO datacube and spectra of UGC 10214

DOI

Minor mergers play a crucial role in galaxy evolution. UGC 10214 (the Tadpole galaxy) is a prime example of this process in which a dwarf galaxy has interacted with a large spiral galaxy ~250 Myr ago and produced a perturbed disc and a giant tidal tail. We used a multi-wavelength dataset that partly consists of new observations (H{alpha}, HI, and CO) and partly of archival data to study the present and past star formation rate (SFR) and its relation to the gas and stellar mass at a spatial resolution down to 4 kpc. UGC 10214 is a high-mass (stellar mass M_=1.28x10^11^ M{sun}) galaxy with a low gas fraction (M_gas/M_=0.24), a high molecular gas fraction (M_H2/M_HI_=0.4), and a modest SFR (2-5 M_{sun}_/yr). The global SFR compared to its stellar mass places UGC 10214 on the galaxy main sequence (MS). The comparison of the molecular gas mass and current SFR gives a molecular gas depletion time of about ~2 Gyr (based on H{alpha}), comparable to those of normal spiral galaxies. Both from a comparison of the H{alpha} emission, tracing the current SFR, and far-ultraviolet (FUV) emission, tracing the recent SFR during the past tens of Myr, and also from spectral energy distribution fitting with CIGALE, we find that the SFR has increased by a factor of about 2-3 during the recent past. This increase is particularly noticeable in the centre of the galaxy where a pronounced peak of the H{alpha} emission is visible. A pixel-to-pixel comparison of the SFR, molecular gas mass, and stellar mass shows that the central region has had a depressed FUV-traced SFR compared to the molecular gas and the stellar mass, whereas the H{alpha}-traced SFR shows a normal level. The atomic and molecular gas distribution is asymmetric, but the position-velocity diagram along the major axis shows a pattern of regular rotation. We conclude that the minor merger has most likely caused variations in the SFR in the past that resulted in a moderate increase of the SFR, but it has not perturbed the gas significantly so that the molecular depletion time remains normal.

Cone search capability for table J/A+A/623/A154/spco10 (List of CO(1-0) spectra of the disk of UGC 10214)

Cone search capability for table J/A+A/623/A154/spco21 (List of CO(2-1) spectra of the disk of UGC 10214)

Cone search capability for table J/A+A/623/A154/list (List of fits files)

Associated data

Identifier
DOI http://doi.org/10.26093/cds/vizier.36230154
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/623/A154
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/623/A154
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/623/A154
Related Identifier https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/A+A/623/A154
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/623/A154
Provenance
Creator Rosado-Belza D.; Lisenfeld U.; Hibbard J.; Kniermann K.; Ott J.; Verley S.,Boquien M.; Jarrett T.; Xu C.K.
Publisher CDS
Publication Year 2019
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Interdisciplinary Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics