Modelling the baryon cycle in low-mass galaxy encounters: the case of NGC 4490 and NGC 4485
ABSTRACT. Discoveries of low-mass galaxy pairs and groups are increasing. Studies indicate that dwarf galaxy pairs are gas rich in the field and exhibit elevat
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 August 3
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 480, Heft: 3, Pages: 3069-3090 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2052 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2052 Verlag, Volltext: https://academic.oup.com/mnras/article/480/3/3069/5066181 
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| Verfasserangaben: | Sarah Pearson, George C. Privon, Gurtina Besla, Mary E. Putman, David Martínez-Delgado, Kathryn V. Johnston, R. Jay Gabany, David R. Patton and Nitya Kallivayalil |
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| 245 | 1 | 0 | |a Modelling the baryon cycle in low-mass galaxy encounters |b the case of NGC 4490 and NGC 4485 |c Sarah Pearson, George C. Privon, Gurtina Besla, Mary E. Putman, David Martínez-Delgado, Kathryn V. Johnston, R. Jay Gabany, David R. Patton and Nitya Kallivayalil |
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| 520 | |a ABSTRACT. Discoveries of low-mass galaxy pairs and groups are increasing. Studies indicate that dwarf galaxy pairs are gas rich in the field and exhibit elevat | ||
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