HALOGAS observations of NGC 4414: fountains, interaction, and ram pressure
| dc.contributor.author | de Blok, W J G | |
| dc.contributor.author | Józsa, G I G | |
| dc.contributor.author | Patterson, M | |
| dc.contributor.author | Gentile, G | |
| dc.contributor.author | Heald, G H | |
| dc.contributor.author | JYtte, E | |
| dc.contributor.author | Kamphuis, P | |
| dc.contributor.author | Rand, R J | |
| dc.contributor.author | Serra, P | |
| dc.contributor.author | Walterbos, R A M | |
| dc.date.accessioned | 2021-10-08T11:01:12Z | |
| dc.date.available | 2021-10-08T11:01:12Z | |
| dc.date.issued | 2014 | |
| dc.description.abstract | We present deep H I imaging of the nearby spiral galaxy NGC 4414, taken as part of the Westerbork HALOGAS (Hydrogen Accretion in LOcal GAlaxieS) survey. The observations show that NGC 4414 can be characterized by a regularly rotating inner H I disk, and a more disturbed outer disk. Modeling of the kinematics shows that the outer disk is best described by a U-shaped warp. Deep optical imaging also reveals the presence of a low surface brightness stellar shell, indicating a minor interaction with a dwarf galaxy at some stage in the past. Modeling of the inner disk suggests that about 4 percent of the inner H I is in the form of extra-planar gas. Because of the disturbed nature of the outer disk, this number is difficult to constrain for the galaxy as a whole. These new, deep observations of NGC 4414 presented here show that even apparently undisturbed galaxies are interacting with their environment. | |
| dc.identifier.apacitation | de Blok, W. J. G., Józsa, G. I. G., Patterson, M., Gentile, G., Heald, G. H., JYtte, E., ... Walterbos, R. A. M. (2014). HALOGAS observations of NGC 4414: fountains, interaction, and ram pressure. <i>Astronomy and Astrophysics</i>, 566(4), A80 - 177. http://hdl.handle.net/11427/35105 | en_ZA |
| dc.identifier.chicagocitation | de Blok, W J G, G I G Józsa, M Patterson, G Gentile, G H Heald, E JYtte, P Kamphuis, R J Rand, P Serra, and R A M Walterbos "HALOGAS observations of NGC 4414: fountains, interaction, and ram pressure." <i>Astronomy and Astrophysics</i> 566, 4. (2014): A80 - 177. http://hdl.handle.net/11427/35105 | en_ZA |
| dc.identifier.citation | de Blok, W.J.G., Józsa, G.I.G., Patterson, M., Gentile, G., Heald, G.H., JYtte, E., Kamphuis, P. & Rand, R.J. et al. 2014. HALOGAS observations of NGC 4414: fountains, interaction, and ram pressure. <i>Astronomy and Astrophysics.</i> 566(4):A80 - 177. http://hdl.handle.net/11427/35105 | en_ZA |
| dc.identifier.issn | 0004-6361 | |
| dc.identifier.issn | 1432-0746 | |
| dc.identifier.ris | TY - Journal Article AU - de Blok, W J G AU - Józsa, G I G AU - Patterson, M AU - Gentile, G AU - Heald, G H AU - JYtte, E AU - Kamphuis, P AU - Rand, R J AU - Serra, P AU - Walterbos, R A M AB - We present deep H I imaging of the nearby spiral galaxy NGC 4414, taken as part of the Westerbork HALOGAS (Hydrogen Accretion in LOcal GAlaxieS) survey. The observations show that NGC 4414 can be characterized by a regularly rotating inner H I disk, and a more disturbed outer disk. Modeling of the kinematics shows that the outer disk is best described by a U-shaped warp. Deep optical imaging also reveals the presence of a low surface brightness stellar shell, indicating a minor interaction with a dwarf galaxy at some stage in the past. Modeling of the inner disk suggests that about 4 percent of the inner H I is in the form of extra-planar gas. Because of the disturbed nature of the outer disk, this number is difficult to constrain for the galaxy as a whole. These new, deep observations of NGC 4414 presented here show that even apparently undisturbed galaxies are interacting with their environment. DA - 2014 DB - OpenUCT DP - University of Cape Town IS - 4 J1 - Astronomy and Astrophysics LK - https://open.uct.ac.za PY - 2014 SM - 0004-6361 SM - 1432-0746 T1 - HALOGAS observations of NGC 4414: fountains, interaction, and ram pressure TI - HALOGAS observations of NGC 4414: fountains, interaction, and ram pressure UR - http://hdl.handle.net/11427/35105 ER - | en_ZA |
| dc.identifier.uri | http://hdl.handle.net/11427/35105 | |
| dc.identifier.vancouvercitation | de Blok WJG, Józsa GIG, Patterson M, Gentile G, Heald GH, JYtte E, et al. HALOGAS observations of NGC 4414: fountains, interaction, and ram pressure. Astronomy and Astrophysics. 2014;566(4):A80 - 177. http://hdl.handle.net/11427/35105. | 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 | 566 | |
| dc.source.pagination | A80 - 177 | |
| dc.source.uri | https://dx.doi.org/10.1051/0004-6361/201322517 | |
| dc.subject.other | Physics and Astronomy | |
| dc.subject.other | galaxies: ISM | |
| dc.subject.other | galaxies: halos | |
| dc.subject.other | galaxies: kinematics and dynamics | |
| dc.subject.other | galaxies: individual: NGC 4414 | |
| dc.subject.other | galaxies: structure | |
| dc.subject.other | ISOLATED SPIRAL NGC-4414 | |
| dc.subject.other | SHELL GALAXIES | |
| dc.subject.other | DISK GALAXIES | |
| dc.subject.other | DARK-MATTER | |
| dc.subject.other | H I | |
| dc.subject.other | GAS | |
| dc.subject.other | LOPSIDEDNESS | |
| dc.subject.other | THINGS | |
| dc.subject.other | MASS | |
| dc.subject.other | POTENTIALS | |
| dc.title | HALOGAS observations of NGC 4414: fountains, interaction, and ram pressure | |
| dc.type | Journal Article | |
| uct.type.publication | Research | |
| uct.type.resource | Journal Article |
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