A study of the nearby interacting galaxy pair NGC 1512/1510
>Magister Scientiae - MSc === This work focuses on generating a new dynamical model of the nearby (9.5 Mpc) interacting galaxy system NGC 1512/1510. Neutral hydrogen (H i ) observations from the Australia Telescope Compact Array (ATCA) are used to model the dynamics of the main H i disk using...
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University of Western Cape
2020
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Online Access: | http://hdl.handle.net/11394/7720 |
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ndltd-netd.ac.za-oai-union.ndltd.org-uwc-oai-etd.uwc.ac.za-11394-77202020-12-11T05:10:57Z A study of the nearby interacting galaxy pair NGC 1512/1510 Ndaliso, Xola Elson, Ed Glowacki, M. Maartens, R. Neutral hydrogen Australia ROTCUR NGC 1512 NGC 1510 >Magister Scientiae - MSc This work focuses on generating a new dynamical model of the nearby (9.5 Mpc) interacting galaxy system NGC 1512/1510. Neutral hydrogen (H i ) observations from the Australia Telescope Compact Array (ATCA) are used to model the dynamics of the main H i disk using two routines, the two and three-dimensional modeling techniques. For the two-dimensional modeling technique, we adopt ROTCUR which is based on fitting a tilted ring model onto the 2D velocity field of the galaxy. The three-dimensional modeling routine used is 3DBarolo, which is a recently developed algorithm of fitting 3D tilted ring model to the full data cube. We note that the 2D approach fails to model the inclination profile of NGC 1512. Thus, a new rotation curve is generated using the three-dimensional modeling routine only i.e. by fitting a 3D tilted ring model to the H i line data cube of NGC 1512/1510. 2020-12-09T12:35:18Z 2020-12-09T12:35:18Z 2020 http://hdl.handle.net/11394/7720 en University of Western Cape University of Western Cape |
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Neutral hydrogen Australia ROTCUR NGC 1512 NGC 1510 |
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Neutral hydrogen Australia ROTCUR NGC 1512 NGC 1510 Ndaliso, Xola A study of the nearby interacting galaxy pair NGC 1512/1510 |
description |
>Magister Scientiae - MSc === This work focuses on generating a new dynamical model of the nearby (9.5 Mpc) interacting
galaxy system NGC 1512/1510. Neutral hydrogen (H i ) observations from the Australia
Telescope Compact Array (ATCA) are used to model the dynamics of the main H i disk using
two routines, the two and three-dimensional modeling techniques. For the two-dimensional
modeling technique, we adopt ROTCUR which is based on fitting a tilted ring model onto
the 2D velocity field of the galaxy. The three-dimensional modeling routine used is 3DBarolo,
which is a recently developed algorithm of fitting 3D tilted ring model to the full data cube.
We note that the 2D approach fails to model the inclination profile of NGC 1512. Thus, a new
rotation curve is generated using the three-dimensional modeling routine only i.e. by fitting a
3D tilted ring model to the H i line data cube of NGC 1512/1510. |
author2 |
Elson, Ed |
author_facet |
Elson, Ed Ndaliso, Xola |
author |
Ndaliso, Xola |
author_sort |
Ndaliso, Xola |
title |
A study of the nearby interacting galaxy pair NGC 1512/1510 |
title_short |
A study of the nearby interacting galaxy pair NGC 1512/1510 |
title_full |
A study of the nearby interacting galaxy pair NGC 1512/1510 |
title_fullStr |
A study of the nearby interacting galaxy pair NGC 1512/1510 |
title_full_unstemmed |
A study of the nearby interacting galaxy pair NGC 1512/1510 |
title_sort |
study of the nearby interacting galaxy pair ngc 1512/1510 |
publisher |
University of Western Cape |
publishDate |
2020 |
url |
http://hdl.handle.net/11394/7720 |
work_keys_str_mv |
AT ndalisoxola astudyofthenearbyinteractinggalaxypairngc15121510 AT ndalisoxola studyofthenearbyinteractinggalaxypairngc15121510 |
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1719370304719945728 |