Sökning: id:"swepub:oai:research.chalmers.se:dd133d6e-74b9-4187-94ba-aaff8a920abc" >
(Sub)millimeter emi...
(Sub)millimeter emission lines of molecules in born-again stars
-
- Tafoya Martinez, Daniel, 1981 (författare)
- Chalmers tekniska högskola,Chalmers University of Technology
-
- Toala, J. A. (författare)
- Academia Sinica Taiwan
-
- Vlemmings, Wouter, 1974 (författare)
- Chalmers tekniska högskola,Chalmers University of Technology
-
visa fler...
-
- Guerrero, M. A. (författare)
- Instituto de Astrofisica de Andalucía (IAA),Institute of Astrophysics of Andalusia (IAA)
-
- De Beck, Elvire, 1985 (författare)
- Chalmers tekniska högskola,Chalmers University of Technology
-
- Gonzalez, M. (författare)
- Instituto de Astrofisica de Andalucía (IAA),Institute of Astrophysics of Andalusia (IAA)
-
- Kimeswenger, S. (författare)
- University of Innsbruck,Universidad Catolica del Norte
-
- Zijlstra, A. (författare)
- University of Manchester
-
- Sanchez-Monge, A. (författare)
- Universität zu Köln,University of Cologne
-
- Treviño Morales, Sandra, 1985 (författare)
- CSIC - Instituto de Ciencia de Materiales de Madrid (ICMM),Observatorio Astronómico Nacional (OAN),Spanish National Observatory (OAN)
-
visa färre...
-
(creator_code:org_t)
- 2017-03-22
- 2017
- Engelska.
-
Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 600
- Relaterad länk:
-
http://publications.... (primary) (free)
-
visa fler...
-
https://www.aanda.or...
-
https://doi.org/10.1...
-
https://research.cha...
-
visa färre...
Abstract
Ämnesord
Stäng
- Context. Born-again stars provide a unique possibility to study the evolution of the circumstellar envelope of evolved stars in human timescales. Up until now, most of the observations of the circumstellar material in these stars have been limited to studying the relatively hot gas and dust. In other evolved stars, the emission from rotational transitions of molecules, such as CO, is commonly used to study the cool component of their circumstellar envelopes. Thus, the detection and study of molecular gas in born-again stars is of great importance when attempting to understand their composition and chemical evolution. In addition, the molecular emission is an invaluable tool for exploring the physical conditions, kinematics, and formation of asymmetric structures in the circumstellar envelopes of these evolved stars. However, up until now, all attempts to detect molecular emission from the cool material around born-again stars have failed. Aims. We searched for emission from rotational transitions of molecules in the hydrogen-deficient circumstellar envelopes of born-again stars to explore the chemical composition, kinematics, and physical parameters of the relatively cool gas. Methods. We carried out observations using the APEX and IRAM 30 m telescopes to search for molecular emission toward four well-studied born-again stars, V4334 Sgr, V605 Aql, A30, and A78, that are thought to represent an evolutionary sequence. Results. For the first time, we detected emission from HCN and (IICN)-C-13 molecules toward V4334 Sgr, and CO emission in V605 Aql. No molecular emission was detected above the noise level toward A30 and A78. The detected lines exhibit broad linewidths greater than or similar to 150 km s(-1), which indicates that the emission comes from gas ejected during the born-again event, rather than from the old planetary nebula. A first estimate of the (HCN)-C-12/(HCN)-C-13 abundance ratio in the circumstellar environment of V4334 Sgr is approximate to 3, which is similar to the value of the C-12/C-13 ratio measured from other observations. We derived a rotational temperature of T-rot = 13 +/- 1 K, and a total column density of N-HCN = 1.6 +/- 0.1 x 10(16) cm(-2) for V4334 Sgr. This result sets a lower limit on the amount of hydrogen that was ejected into the wind during the born-again event of this source. For V605 Aql, we obtained a lower limit for the integrated line intensities I-12CO/I-13CO > 4.
Ämnesord
- NATURVETENSKAP -- Fysik -- Den kondenserade materiens fysik (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Condensed Matter Physics (hsv//eng)
Nyckelord
- stars: carbon
- planetary nebulae: general
- stars: AGB and post-AGB
- circumstellar matter
- stars: mass-loss
Publikations- och innehållstyp
- art (ämneskategori)
- ref (ämneskategori)
Hitta via bibliotek
Till lärosätets databas
- Av författaren/redakt...
-
Tafoya Martinez, ...
-
Toala, J. A.
-
Vlemmings, Woute ...
-
Guerrero, M. A.
-
De Beck, Elvire, ...
-
Gonzalez, M.
-
visa fler...
-
Kimeswenger, S.
-
Zijlstra, A.
-
Sanchez-Monge, A ...
-
Treviño Morales, ...
-
visa färre...
- Om ämnet
-
- NATURVETENSKAP
-
NATURVETENSKAP
-
och Fysik
-
och Den kondenserade ...
- Artiklar i publikationen
-
Astronomy and As ...
- Av lärosätet
-
Chalmers tekniska högskola