[Fe iii] lines in the planetary nebula NGC 2392
The Eskimo Nebula (NGC 2392) is a young double-shell planetary nebula (PN). Its intrinsic structure and the responsible shaping mechanism are still not fully understood. We present new optical spectroscopy of NGC 2392 at two different locations to obtain the spectra of the inner and outer shells. Se...
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Online Access: | https://doi.org/10.1017/S1743921312012288 http://hdl.handle.net/10722/165696 |
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ftunivhongkonghu:oai:hub.hku.hk:10722/165696 2023-05-15T16:07:03+02:00 [Fe iii] lines in the planetary nebula NGC 2392 Fang, X Hsia, CH Liu, XW Chau, WC Kwok, S Zhang, Y 2011 https://doi.org/10.1017/S1743921312012288 http://hdl.handle.net/10722/165696 eng eng Cambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU United Kingdom International Astronomical Union Proceedings IAU Symposium No. 283: Planetary Nebulae: An Eye to the Future, Puerto de la Cruz, Tenerife, Spain, 25-29 July 2011. In International Astronomical Union Proceedings, 2011, v. 7 n. S283, p. 532-533 doi:10.1017/S1743921312012288 533 209392 WOS:000309944800169 1743-9213 S283 eid_2-s2.0-84865705257 532 http://hdl.handle.net/10722/165696 7 International Astronomical Union Proceedings. Copyright © Cambridge University Press. This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License. CC-BY-NC-ND line: identification planetary nebulae: individual (NGC 2392 Mz 3) Conference_Paper 2011 ftunivhongkonghu https://doi.org/10.1017/S1743921312012288 2023-01-14T15:49:03Z The Eskimo Nebula (NGC 2392) is a young double-shell planetary nebula (PN). Its intrinsic structure and the responsible shaping mechanism are still not fully understood. We present new optical spectroscopy of NGC 2392 at two different locations to obtain the spectra of the inner and outer shells. Several [Fe iii] lines are clearly detected. We find that these [Fe iii] lines mostly originate from the inner shell. Therefore, we suggest that NGC 2392 might have an intrinsic structure similar to the Ant Nebula Mz 3, which exhibits a number of [Fe iii] lines from the central dense regions. In this scenario, the inner and outer shells correspond to the central emission core and the outer lobes of Mz 3, respectively. © 2012 International Astronomical Union. published_or_final_version Conference Object eskimo* University of Hong Kong: HKU Scholars Hub Proceedings of the International Astronomical Union 7 S283 532 533 |
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University of Hong Kong: HKU Scholars Hub |
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ftunivhongkonghu |
language |
English |
topic |
line: identification planetary nebulae: individual (NGC 2392 Mz 3) |
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line: identification planetary nebulae: individual (NGC 2392 Mz 3) Fang, X Hsia, CH Liu, XW Chau, WC Kwok, S Zhang, Y [Fe iii] lines in the planetary nebula NGC 2392 |
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line: identification planetary nebulae: individual (NGC 2392 Mz 3) |
description |
The Eskimo Nebula (NGC 2392) is a young double-shell planetary nebula (PN). Its intrinsic structure and the responsible shaping mechanism are still not fully understood. We present new optical spectroscopy of NGC 2392 at two different locations to obtain the spectra of the inner and outer shells. Several [Fe iii] lines are clearly detected. We find that these [Fe iii] lines mostly originate from the inner shell. Therefore, we suggest that NGC 2392 might have an intrinsic structure similar to the Ant Nebula Mz 3, which exhibits a number of [Fe iii] lines from the central dense regions. In this scenario, the inner and outer shells correspond to the central emission core and the outer lobes of Mz 3, respectively. © 2012 International Astronomical Union. published_or_final_version |
format |
Conference Object |
author |
Fang, X Hsia, CH Liu, XW Chau, WC Kwok, S Zhang, Y |
author_facet |
Fang, X Hsia, CH Liu, XW Chau, WC Kwok, S Zhang, Y |
author_sort |
Fang, X |
title |
[Fe iii] lines in the planetary nebula NGC 2392 |
title_short |
[Fe iii] lines in the planetary nebula NGC 2392 |
title_full |
[Fe iii] lines in the planetary nebula NGC 2392 |
title_fullStr |
[Fe iii] lines in the planetary nebula NGC 2392 |
title_full_unstemmed |
[Fe iii] lines in the planetary nebula NGC 2392 |
title_sort |
[fe iii] lines in the planetary nebula ngc 2392 |
publisher |
Cambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU |
publishDate |
2011 |
url |
https://doi.org/10.1017/S1743921312012288 http://hdl.handle.net/10722/165696 |
genre |
eskimo* |
genre_facet |
eskimo* |
op_relation |
International Astronomical Union Proceedings IAU Symposium No. 283: Planetary Nebulae: An Eye to the Future, Puerto de la Cruz, Tenerife, Spain, 25-29 July 2011. In International Astronomical Union Proceedings, 2011, v. 7 n. S283, p. 532-533 doi:10.1017/S1743921312012288 533 209392 WOS:000309944800169 1743-9213 S283 eid_2-s2.0-84865705257 532 http://hdl.handle.net/10722/165696 7 |
op_rights |
International Astronomical Union Proceedings. Copyright © Cambridge University Press. This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License. |
op_rightsnorm |
CC-BY-NC-ND |
op_doi |
https://doi.org/10.1017/S1743921312012288 |
container_title |
Proceedings of the International Astronomical Union |
container_volume |
7 |
container_issue |
S283 |
container_start_page |
532 |
op_container_end_page |
533 |
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1766403063862525952 |