Isolated and non-isolated dwarfs in terms of modified Newtonian dynamics
| dc.contributor.author | Gentile, G | |
| dc.contributor.author | Angus, G W | |
| dc.contributor.author | Famaey, B | |
| dc.contributor.author | Oh, S-H | |
| dc.contributor.author | de Blok, W J G | |
| dc.date.accessioned | 2021-10-08T11:01:07Z | |
| dc.date.available | 2021-10-08T11:01:07Z | |
| dc.date.issued | 2012 | |
| dc.description.abstract | Within the framework of modified Newtonian dynamics (MOND), we investigate the kinematics of two dwarf spiral galaxies belonging to very different environments, namely KK 246 in the Local Void and Holmberg II in the M 81 group. A mass model of the rotation curve of KK 246 is presented for the first time, and we show that its observed kinematics are consistent with MOND. We re-derive the outer rotation curve of Holmberg II, by modelling its HI data cube, and find that its inclination should be closer to face-on than previously derived. This implies that Holmberg II has a higher rotation velocity in its outer parts, which, although not very precisely constrained, is consistent with the MOND prediction. | |
| dc.identifier.apacitation | Gentile, G., Angus, G. W., Famaey, B., Oh, S., & de Blok, W. J. G. (2012). Isolated and non-isolated dwarfs in terms of modified Newtonian dynamics. <i>Astronomy and Astrophysics</i>, 543(4), A47 - 177. http://hdl.handle.net/11427/35089 | en_ZA |
| dc.identifier.chicagocitation | Gentile, G, G W Angus, B Famaey, S-H Oh, and W J G de Blok "Isolated and non-isolated dwarfs in terms of modified Newtonian dynamics." <i>Astronomy and Astrophysics</i> 543, 4. (2012): A47 - 177. http://hdl.handle.net/11427/35089 | en_ZA |
| dc.identifier.citation | Gentile, G., Angus, G.W., Famaey, B., Oh, S. & de Blok, W.J.G. 2012. Isolated and non-isolated dwarfs in terms of modified Newtonian dynamics. <i>Astronomy and Astrophysics.</i> 543(4):A47 - 177. http://hdl.handle.net/11427/35089 | en_ZA |
| dc.identifier.issn | 0004-6361 | |
| dc.identifier.issn | 1432-0746 | |
| dc.identifier.ris | TY - Journal Article AU - Gentile, G AU - Angus, G W AU - Famaey, B AU - Oh, S-H AU - de Blok, W J G AB - Within the framework of modified Newtonian dynamics (MOND), we investigate the kinematics of two dwarf spiral galaxies belonging to very different environments, namely KK 246 in the Local Void and Holmberg II in the M 81 group. A mass model of the rotation curve of KK 246 is presented for the first time, and we show that its observed kinematics are consistent with MOND. We re-derive the outer rotation curve of Holmberg II, by modelling its HI data cube, and find that its inclination should be closer to face-on than previously derived. This implies that Holmberg II has a higher rotation velocity in its outer parts, which, although not very precisely constrained, is consistent with the MOND prediction. DA - 2012 DB - OpenUCT DP - University of Cape Town IS - 4 J1 - Astronomy and Astrophysics LK - https://open.uct.ac.za PY - 2012 SM - 0004-6361 SM - 1432-0746 T1 - Isolated and non-isolated dwarfs in terms of modified Newtonian dynamics TI - Isolated and non-isolated dwarfs in terms of modified Newtonian dynamics UR - http://hdl.handle.net/11427/35089 ER - | en_ZA |
| dc.identifier.uri | http://hdl.handle.net/11427/35089 | |
| dc.identifier.vancouvercitation | Gentile G, Angus GW, Famaey B, Oh S, de Blok WJG. Isolated and non-isolated dwarfs in terms of modified Newtonian dynamics. Astronomy and Astrophysics. 2012;543(4):A47 - 177. http://hdl.handle.net/11427/35089. | en_ZA |
| dc.language.iso | eng | |
| dc.publisher.department | Department of Astronomy | |
| dc.publisher.faculty | Faculty of Science | |
| dc.source | Astronomy and Astrophysics | |
| dc.source.journalissue | 4 | |
| dc.source.journalvolume | 543 | |
| dc.source.pagination | A47 - 177 | |
| dc.source.uri | https://dx.doi.org/10.1051/0004-6361/201218997 | |
| dc.subject.other | Physics and Astronomy | |
| dc.subject.other | dark matter | |
| dc.subject.other | galaxies: kinematics and dynamics | |
| dc.subject.other | galaxies: dwarf | |
| dc.subject.other | gravitation | |
| dc.subject.other | HOLMBERG-II | |
| dc.subject.other | GALAXIES | |
| dc.subject.other | DARK | |
| dc.subject.other | MATTER | |
| dc.subject.other | DISK | |
| dc.subject.other | MASS | |
| dc.subject.other | DENSITY | |
| dc.title | Isolated and non-isolated dwarfs in terms of modified Newtonian dynamics | |
| dc.type | Journal Article | |
| uct.type.publication | Research | |
| uct.type.resource | Journal Article |
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