Spiral-shells and nascent bipolar outflow in CIT 6: Hints for an eccentric-orbit binary?

Hyosun Kim; Sheng Yuan Liu; Naomi Hirano; Ronny Zhao-Geisler; Alfonso Trejo; Hsi Wei Yen; Ronald E. Taam; Francisca Kemper; Jongsoo Kim; Do Young Byun; Tie Liu

doi:10.1088/1742-6596/728/7/072018

Spiral-shells and nascent bipolar outflow in CIT 6: Hints for an eccentric-orbit binary?

Hyosun Kim, Sheng Yuan Liu, Naomi Hirano, Ronny Zhao-Geisler, Alfonso Trejo, Hsi Wei Yen, Ronald E. Taam, Francisca Kemper, Jongsoo Kim, Do Young Byun, Tie Liu

Physics and Astronomy

Research output: Contribution to journal › Conference article › peer-review

Abstract

We present the essential results pointed out in a recently published paper, Kim et al. 2015, Astrophys. J., 814, 61. The carbon star CIT 6 reveals evidences for a binary in a high-resolution CO line emission map of its circumstellar envelope taken with the Submillimeter Array. The morphology of the outflow described by the spiral-shell pattern, bipolar (or possibly multipolar) outflow, one-sided interarm gaps, and double spiral feature point to a plausible scenario that CIT 6 is a binary system in an eccentric orbit with the mass losing star evolving from the AGB.

Original language	English (US)
Article number	072018
Journal	Journal of Physics: Conference Series
Volume	728
Issue number	7
DOIs	https://doi.org/10.1088/1742-6596/728/7/072018
State	Published - Aug 8 2016
Event	11th Pacific Rim Conference on Stellar Astrophysics: Physics and Chemistry of the Late Stages of Stellar Evolution - Hong Kong, China Duration: Dec 14 2015 → Dec 17 2015

ASJC Scopus subject areas

Physics and Astronomy(all)

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10.1088/1742-6596/728/7/072018

Cite this

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title = "Spiral-shells and nascent bipolar outflow in CIT 6: Hints for an eccentric-orbit binary?",

abstract = "We present the essential results pointed out in a recently published paper, Kim et al. 2015, Astrophys. J., 814, 61. The carbon star CIT 6 reveals evidences for a binary in a high-resolution CO line emission map of its circumstellar envelope taken with the Submillimeter Array. The morphology of the outflow described by the spiral-shell pattern, bipolar (or possibly multipolar) outflow, one-sided interarm gaps, and double spiral feature point to a plausible scenario that CIT 6 is a binary system in an eccentric orbit with the mass losing star evolving from the AGB.",

author = "Hyosun Kim and Liu, {Sheng Yuan} and Naomi Hirano and Ronny Zhao-Geisler and Alfonso Trejo and Yen, {Hsi Wei} and Taam, {Ronald E.} and Francisca Kemper and Jongsoo Kim and Byun, {Do Young} and Tie Liu",

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language = "English (US)",

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TY - JOUR

T1 - Spiral-shells and nascent bipolar outflow in CIT 6

T2 - 11th Pacific Rim Conference on Stellar Astrophysics: Physics and Chemistry of the Late Stages of Stellar Evolution

AU - Kim, Hyosun

AU - Liu, Sheng Yuan

AU - Hirano, Naomi

AU - Zhao-Geisler, Ronny

AU - Trejo, Alfonso

AU - Yen, Hsi Wei

AU - Taam, Ronald E.

AU - Kemper, Francisca

AU - Kim, Jongsoo

AU - Byun, Do Young

AU - Liu, Tie

PY - 2016/8/8

Y1 - 2016/8/8

N2 - We present the essential results pointed out in a recently published paper, Kim et al. 2015, Astrophys. J., 814, 61. The carbon star CIT 6 reveals evidences for a binary in a high-resolution CO line emission map of its circumstellar envelope taken with the Submillimeter Array. The morphology of the outflow described by the spiral-shell pattern, bipolar (or possibly multipolar) outflow, one-sided interarm gaps, and double spiral feature point to a plausible scenario that CIT 6 is a binary system in an eccentric orbit with the mass losing star evolving from the AGB.

AB - We present the essential results pointed out in a recently published paper, Kim et al. 2015, Astrophys. J., 814, 61. The carbon star CIT 6 reveals evidences for a binary in a high-resolution CO line emission map of its circumstellar envelope taken with the Submillimeter Array. The morphology of the outflow described by the spiral-shell pattern, bipolar (or possibly multipolar) outflow, one-sided interarm gaps, and double spiral feature point to a plausible scenario that CIT 6 is a binary system in an eccentric orbit with the mass losing star evolving from the AGB.

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DO - 10.1088/1742-6596/728/7/072018

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SN - 1742-6588

VL - 728

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

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M1 - 072018

Y2 - 14 December 2015 through 17 December 2015

ER -

Spiral-shells and nascent bipolar outflow in CIT 6: Hints for an eccentric-orbit binary?

Abstract

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