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Article: Bima CO observation of EP aquarii: The semiregular pulsating star with a double-component line profile
Title | Bima CO observation of EP aquarii: The semiregular pulsating star with a double-component line profile |
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Authors | |
Keywords | Circumstellar Matter Stars: Agb And Post-Agb Stars: Imaging Stars: Individual (Ep Aquarii) Stars: Late-Type Stars: Mass Loss |
Issue Date | 2006 |
Publisher | Institute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205 |
Citation | Astrophysical Journal Letters, 2006, v. 638 n. 2 I, p. 1041-1044 How to Cite? |
Abstract | This paper reports the results of a Berkeley-Illinois-Maryland Association array interferometric observation of EP Aqr, a semiregular pulsating star with a double-component line profile in the CO J = 1-0 line. The broad component shows a flat-topped profile, and the narrow component shows a spiky strong peak. Although previous single-dish observations suggested that the CO J = 2-1 line exhibits a Gaussian-like profile, the CO J = 1-0 line does not. The spatial distributions of both the narrow and the broad components appear to be roughly round with the same peak positions. No significant velocity gradient is seen. The spatial-kinetic properties of the molecular envelope of EP Aqr are reminiscent of a multiple-shell structure model rather than of a bipolar flow and disk model. A problem with this interpretation is that no evidence of interaction between the narrow- and broad-component regions is seen. A Gaussian-like feature seen in the CO J = 2-1 line might play a key role in understanding the spatiokinetic properties of the molecular envelope of EP Aqr. © 2006. The American Astronomical Society. All rights reserved. |
Persistent Identifier | http://hdl.handle.net/10722/175003 |
ISSN | 2023 Impact Factor: 8.8 2023 SCImago Journal Rankings: 2.766 |
ISI Accession Number ID | |
References |
DC Field | Value | Language |
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dc.contributor.author | Nakashima, JI | en_US |
dc.date.accessioned | 2012-11-26T08:48:44Z | - |
dc.date.available | 2012-11-26T08:48:44Z | - |
dc.date.issued | 2006 | en_US |
dc.identifier.citation | Astrophysical Journal Letters, 2006, v. 638 n. 2 I, p. 1041-1044 | en_US |
dc.identifier.issn | 2041-8205 | en_US |
dc.identifier.uri | http://hdl.handle.net/10722/175003 | - |
dc.description.abstract | This paper reports the results of a Berkeley-Illinois-Maryland Association array interferometric observation of EP Aqr, a semiregular pulsating star with a double-component line profile in the CO J = 1-0 line. The broad component shows a flat-topped profile, and the narrow component shows a spiky strong peak. Although previous single-dish observations suggested that the CO J = 2-1 line exhibits a Gaussian-like profile, the CO J = 1-0 line does not. The spatial distributions of both the narrow and the broad components appear to be roughly round with the same peak positions. No significant velocity gradient is seen. The spatial-kinetic properties of the molecular envelope of EP Aqr are reminiscent of a multiple-shell structure model rather than of a bipolar flow and disk model. A problem with this interpretation is that no evidence of interaction between the narrow- and broad-component regions is seen. A Gaussian-like feature seen in the CO J = 2-1 line might play a key role in understanding the spatiokinetic properties of the molecular envelope of EP Aqr. © 2006. The American Astronomical Society. All rights reserved. | en_US |
dc.language | eng | en_US |
dc.publisher | Institute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205 | en_US |
dc.relation.ispartof | Astrophysical Journal Letters | en_US |
dc.subject | Circumstellar Matter | en_US |
dc.subject | Stars: Agb And Post-Agb | en_US |
dc.subject | Stars: Imaging | en_US |
dc.subject | Stars: Individual (Ep Aquarii) | en_US |
dc.subject | Stars: Late-Type | en_US |
dc.subject | Stars: Mass Loss | en_US |
dc.title | Bima CO observation of EP aquarii: The semiregular pulsating star with a double-component line profile | en_US |
dc.type | Article | en_US |
dc.identifier.email | Nakashima, JI: junichi@hku.hk | en_US |
dc.identifier.authority | Nakashima, JI=rp00764 | en_US |
dc.description.nature | link_to_subscribed_fulltext | en_US |
dc.identifier.doi | 10.1086/498934 | en_US |
dc.identifier.scopus | eid_2-s2.0-33644813397 | en_US |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-33644813397&selection=ref&src=s&origin=recordpage | en_US |
dc.identifier.volume | 638 | en_US |
dc.identifier.issue | 2 I | en_US |
dc.identifier.spage | 1041 | en_US |
dc.identifier.epage | 1044 | en_US |
dc.identifier.isi | WOS:000235425700042 | - |
dc.publisher.place | United Kingdom | en_US |
dc.identifier.scopusauthorid | Nakashima, JI=35485342300 | en_US |
dc.identifier.issnl | 2041-8205 | - |