Formation of S0s in extreme environments I: clues from kinematics and stellar populations. Issue 2 (28th December 2019)
- Record Type:
- Journal Article
- Title:
- Formation of S0s in extreme environments I: clues from kinematics and stellar populations. Issue 2 (28th December 2019)
- Main Title:
- Formation of S0s in extreme environments I: clues from kinematics and stellar populations
- Authors:
- Coccato, Lodovico
Jaffé, Yara L
Cortesi, Arianna
Merrifield, Michael
Johnston, Evelyn
Rodríguez del Pino, Bruno
Haeussler, Boris
Chies-Santos, Ana L
Mendes de Oliveira, Claudia L
Sheen, Yun-Kyeong
Menéndez-Delmestre, Karín - Abstract:
- ABSTRACT: Despite numerous efforts, it is still unclear whether lenticular galaxies (S0s) evolve from spirals whose star formation was suppressed, or formed trough mergers or disc instabilities. In this paper we present a pilot study of 21 S0 galaxies in extreme environments (field and cluster), and compare their spatially resolved kinematics and global stellar populations. Our aim is to identify whether there are different mechanisms that form S0s in different environments. Our results show that the kinematics of S0 galaxies in field and cluster are, indeed, different. Lenticulars in the cluster are more rotationally supported, suggesting that they are formed through processes that involve the rapid consumption or removal of gas (e.g. starvation, ram pressure stripping). In contrast, S0s in the field are more pressure supported, suggesting that minor mergers served mostly to shape their kinematic properties. These results are independent of total mass, luminosity, or disc-to-bulge ratio. On the other hand, the mass-weighted age, metallicity, and star formation time-scale of the galaxies correlate more with mass than with environment, in agreement with known relations from previous work, such as the one between mass and metallicity. Overall, our results re-enforce the idea that there are multiple mechanisms that produce S0s, and that both mass and environment play key roles. A larger sample is highly desirable to confirm or refute the results and the interpretation of thisABSTRACT: Despite numerous efforts, it is still unclear whether lenticular galaxies (S0s) evolve from spirals whose star formation was suppressed, or formed trough mergers or disc instabilities. In this paper we present a pilot study of 21 S0 galaxies in extreme environments (field and cluster), and compare their spatially resolved kinematics and global stellar populations. Our aim is to identify whether there are different mechanisms that form S0s in different environments. Our results show that the kinematics of S0 galaxies in field and cluster are, indeed, different. Lenticulars in the cluster are more rotationally supported, suggesting that they are formed through processes that involve the rapid consumption or removal of gas (e.g. starvation, ram pressure stripping). In contrast, S0s in the field are more pressure supported, suggesting that minor mergers served mostly to shape their kinematic properties. These results are independent of total mass, luminosity, or disc-to-bulge ratio. On the other hand, the mass-weighted age, metallicity, and star formation time-scale of the galaxies correlate more with mass than with environment, in agreement with known relations from previous work, such as the one between mass and metallicity. Overall, our results re-enforce the idea that there are multiple mechanisms that produce S0s, and that both mass and environment play key roles. A larger sample is highly desirable to confirm or refute the results and the interpretation of this pilot study. … (more)
- Is Part Of:
- Monthly notices of the Royal Astronomical Society. Volume 492:Issue 2(2020)
- Journal:
- Monthly notices of the Royal Astronomical Society
- Issue:
- Volume 492:Issue 2(2020)
- Issue Display:
- Volume 492, Issue 2 (2020)
- Year:
- 2020
- Volume:
- 492
- Issue:
- 2
- Issue Sort Value:
- 2020-0492-0002-0000
- Page Start:
- 2955
- Page End:
- 2972
- Publication Date:
- 2019-12-28
- Subjects:
- galaxies: elliptical and lenticular, cD -- galaxies: formation -- galaxies: kinematics and dynamics
Astronomy -- Periodicals
Periodicals
520.5 - Journal URLs:
- http://mnras.oxfordjournals.org/ ↗
http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966 ↗
http://www.blackwell-synergy.com/issuelist.asp?journal=mnr ↗
http://www.blackwell-synergy.com/loi/mnr ↗
http://ukcatalogue.oup.com/ ↗ - DOI:
- 10.1093/mnras/stz3592 ↗
- Languages:
- English
- ISSNs:
- 0035-8711
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 5943.000000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 12654.xml