File Download
Links for fulltext
(May Require Subscription)
- Publisher Website: 10.1086/306449
- Scopus: eid_2-s2.0-22444453855
- WOS: WOS:000077780500031
- Find via
Supplementary
- Citations:
- Appears in Collections:
Article: Hubble space telescope imaging of iras 17441-2411: A case study of a bipolar nebula with a circumstellar disk
Title | Hubble space telescope imaging of iras 17441-2411: A case study of a bipolar nebula with a circumstellar disk |
---|---|
Authors | |
Keywords | Circumstellar Matter Planetary Nebulae: General Stars: Agb And Post-Agb |
Issue Date | 1998 |
Publisher | Institute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/0004-637X |
Citation | The Astrophysical Journal, 1998, v. 508 n. 2 pt. 2, p. 744-751 How to Cite? |
Abstract | The bipolar proto-planetary nebula IRAS 17441-2411 (the "Silkworm Nebula") was observed with the Hubble Space Telescope. By fitting the observed spectral energy distribution and the V-band image by a two-dimensional radiation transfer model, we derive the properties of the circumstellar wind and a proposed circumstellar "disk." We suggest that bipolar structures are probably more common than actually observed, because objects with similar intrinsic structures may simply appear stellar because of their orientation in the sky. © 1998. The American Astronomical Society. All rights reserved. |
Persistent Identifier | http://hdl.handle.net/10722/179687 |
ISSN | 2023 Impact Factor: 4.8 2023 SCImago Journal Rankings: 1.905 |
ISI Accession Number ID | |
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Su, KYL | en_US |
dc.contributor.author | Volk, K | en_US |
dc.contributor.author | Kwok, S | en_US |
dc.contributor.author | Hrivnak, BJ | en_US |
dc.date.accessioned | 2012-12-19T10:02:50Z | - |
dc.date.available | 2012-12-19T10:02:50Z | - |
dc.date.issued | 1998 | en_US |
dc.identifier.citation | The Astrophysical Journal, 1998, v. 508 n. 2 pt. 2, p. 744-751 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/10722/179687 | - |
dc.description.abstract | The bipolar proto-planetary nebula IRAS 17441-2411 (the "Silkworm Nebula") was observed with the Hubble Space Telescope. By fitting the observed spectral energy distribution and the V-band image by a two-dimensional radiation transfer model, we derive the properties of the circumstellar wind and a proposed circumstellar "disk." We suggest that bipolar structures are probably more common than actually observed, because objects with similar intrinsic structures may simply appear stellar because of their orientation in the sky. © 1998. 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/0004-637X | en_US |
dc.relation.ispartof | The Astrophysical Journal | en_US |
dc.subject | Circumstellar Matter | en_US |
dc.subject | Planetary Nebulae: General | en_US |
dc.subject | Stars: Agb And Post-Agb | en_US |
dc.title | Hubble space telescope imaging of iras 17441-2411: A case study of a bipolar nebula with a circumstellar disk | en_US |
dc.type | Article | en_US |
dc.identifier.email | Kwok, S: deannote@hku.hk | en_US |
dc.identifier.authority | Kwok, S=rp00716 | en_US |
dc.description.nature | published_or_final_version | en_US |
dc.identifier.doi | 10.1086/306449 | en_US |
dc.identifier.scopus | eid_2-s2.0-22444453855 | en_US |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-22444453855&selection=ref&src=s&origin=recordpage | en_US |
dc.identifier.volume | 508 | en_US |
dc.identifier.issue | 2 pt. 2 | en_US |
dc.identifier.spage | 744 | en_US |
dc.identifier.epage | 751 | en_US |
dc.identifier.isi | WOS:000077780500031 | - |
dc.publisher.place | United Kingdom | en_US |
dc.identifier.scopusauthorid | Su, KYL=26326482200 | en_US |
dc.identifier.scopusauthorid | Volk, K=7006571965 | en_US |
dc.identifier.scopusauthorid | Kwok, S=22980498300 | en_US |
dc.identifier.scopusauthorid | Hrivnak, BJ=35613962100 | en_US |
dc.identifier.issnl | 0004-637X | - |