Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s
We use integral field spectroscopy of 13 disc galaxies in the cluster AC114 at z ∼ 0.31 in an attempt to disentangle the physical processes responsible for the transformation of spiral galaxies in clusters. Our sample is selected to display a dominant young stellar population, as indicated by strong...
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| Format: | Article |
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Oxford University Press
2014
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| Online Access: | https://eprints.nottingham.ac.uk/42056/ |
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| author | Rodriguez Del Pino, Bruno Bamford, Steven P. Aragón-Salamanca, Alfonso Milvang-Jensen, Bo Merrifield, Michael R. Balcells, Marc |
| author_facet | Rodriguez Del Pino, Bruno Bamford, Steven P. Aragón-Salamanca, Alfonso Milvang-Jensen, Bo Merrifield, Michael R. Balcells, Marc |
| author_sort | Rodriguez Del Pino, Bruno |
| building | Nottingham Research Data Repository |
| collection | Online Access |
| description | We use integral field spectroscopy of 13 disc galaxies in the cluster AC114 at z ∼ 0.31 in an attempt to disentangle the physical processes responsible for the transformation of spiral galaxies in clusters. Our sample is selected to display a dominant young stellar population, as indicated by strong Hδ absorption lines in their integrated spectra. Most of our galaxies lack the [O ii]λ3727 emission line, and hence ongoing star formation. They therefore possess ‘k+a’ spectra, indicative of a recent truncation of star formation, possibly preceded by a starburst. Discy ‘k+a’ galaxies are a promising candidate for the intermediate stage of the transformation from star-forming spiral galaxies to passive S0s. Our observations allow us to study the spatial distributions and the kinematics of the different stellar populations within the galaxies. We used three different indicators to evaluate the presence of a young population: the equivalent width of Hδ, the luminosity-weighted fraction of A stars, and the fraction of the galaxy light attributable to simple stellar populations with ages between 0.5 and 1.5 Gyr. We find a mixture of behaviours, but are able to show that in most of the galaxies the last episode of star formation occurred in an extended disc, similar to preceding generations of stars, though somewhat more centrally concentrated. We thus exclude nuclear starbursts and violent gravitational interactions as causes of the star formation truncation. Gentler mechanisms, such as ram-pressure stripping or weak galaxy–galaxy interactions, appear to be responsible for ending star formation in these intermediate-redshift cluster disc galaxies. |
| first_indexed | 2025-11-14T19:47:30Z |
| format | Article |
| id | nottingham-42056 |
| institution | University of Nottingham Malaysia Campus |
| institution_category | Local University |
| last_indexed | 2025-11-14T19:47:30Z |
| publishDate | 2014 |
| publisher | Oxford University Press |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | nottingham-420562020-05-04T16:40:57Z https://eprints.nottingham.ac.uk/42056/ Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s Rodriguez Del Pino, Bruno Bamford, Steven P. Aragón-Salamanca, Alfonso Milvang-Jensen, Bo Merrifield, Michael R. Balcells, Marc We use integral field spectroscopy of 13 disc galaxies in the cluster AC114 at z ∼ 0.31 in an attempt to disentangle the physical processes responsible for the transformation of spiral galaxies in clusters. Our sample is selected to display a dominant young stellar population, as indicated by strong Hδ absorption lines in their integrated spectra. Most of our galaxies lack the [O ii]λ3727 emission line, and hence ongoing star formation. They therefore possess ‘k+a’ spectra, indicative of a recent truncation of star formation, possibly preceded by a starburst. Discy ‘k+a’ galaxies are a promising candidate for the intermediate stage of the transformation from star-forming spiral galaxies to passive S0s. Our observations allow us to study the spatial distributions and the kinematics of the different stellar populations within the galaxies. We used three different indicators to evaluate the presence of a young population: the equivalent width of Hδ, the luminosity-weighted fraction of A stars, and the fraction of the galaxy light attributable to simple stellar populations with ages between 0.5 and 1.5 Gyr. We find a mixture of behaviours, but are able to show that in most of the galaxies the last episode of star formation occurred in an extended disc, similar to preceding generations of stars, though somewhat more centrally concentrated. We thus exclude nuclear starbursts and violent gravitational interactions as causes of the star formation truncation. Gentler mechanisms, such as ram-pressure stripping or weak galaxy–galaxy interactions, appear to be responsible for ending star formation in these intermediate-redshift cluster disc galaxies. Oxford University Press 2014-02-01 Article PeerReviewed Rodriguez Del Pino, Bruno, Bamford, Steven P., Aragón-Salamanca, Alfonso, Milvang-Jensen, Bo, Merrifield, Michael R. and Balcells, Marc (2014) Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s. Monthly Notices of the Royal Astronomical Society, 438 (2). pp. 1038-1050. ISSN 0035-8711 galaxies: clusters: individual: AC114 galaxies: evolution galaxies: interactions https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stt2202 doi:10.1093/mnras/stt2202 doi:10.1093/mnras/stt2202 |
| spellingShingle | galaxies: clusters: individual: AC114 galaxies: evolution galaxies: interactions Rodriguez Del Pino, Bruno Bamford, Steven P. Aragón-Salamanca, Alfonso Milvang-Jensen, Bo Merrifield, Michael R. Balcells, Marc Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s |
| title | Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s |
| title_full | Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s |
| title_fullStr | Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s |
| title_full_unstemmed | Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s |
| title_short | Caught in the act: cluster 'k+a' galaxies as a link between spirals and S0s |
| title_sort | caught in the act: cluster 'k+a' galaxies as a link between spirals and s0s |
| topic | galaxies: clusters: individual: AC114 galaxies: evolution galaxies: interactions |
| url | https://eprints.nottingham.ac.uk/42056/ https://eprints.nottingham.ac.uk/42056/ https://eprints.nottingham.ac.uk/42056/ |