Registration of H2O and SiO masers in the Calabash Nebula to confirm the planetary nebula paradigm

R. Dodson, M. Rioja, V. Bujarrabal, J. Kim, S. H. Cho, Y. K. Choix, Y. Youngjoo

Research output: Contribution to journalArticle

2 Citations (Scopus)

Abstract

We report on the astrometric registration of very long baseline interferometry images of the SiO and H2O masers in OH231.8+4.2, the iconic proto-planetary nebula also known as the Calabash nebula, using the Korean VLBI Network and source frequency phase referencing. This, for the first time, robustly confirms the alignment of the SiO masers, close to the asymptotic giant branch star, driving the bilobe structure with the water masers in the outflow. We are able to trace the bulk motions for the H2O masers over the last few decades to be 19 km s-1 and deduce that the age of this expansion stage is 38±2 yr. The combination of this result with the distance allows a full 3D reconstruction and confirms that the H2O masers lie on and expand along the known large-scale symmetry axis and that the outflow is only a few decades old, so mass loss is almost certainly ongoing. Therefore, we conclude that the SiO emission marks the stellar core of the nebular, the H2O emission traces the expansion, and there must be multiple epochs of ejection to drive the macro-scale structure.

Original languageEnglish
Pages (from-to)520-527
Number of pages8
JournalMonthly Notices of the Royal Astronomical Society
Volume476
Issue number1
DOIs
Publication statusPublished - 1 May 2018

Fingerprint

very long baseline interferometry
planetary nebulae
masers
nebulae
outflow
symmetry
water masers
stellar cores
expansion
very long base interferometry
asymptotic giant branch stars
ejection
interferometry
alignment
time measurement
water
registration
loss

Cite this

Dodson, R. ; Rioja, M. ; Bujarrabal, V. ; Kim, J. ; Cho, S. H. ; Choix, Y. K. ; Youngjoo, Y. / Registration of H2O and SiO masers in the Calabash Nebula to confirm the planetary nebula paradigm. In: Monthly Notices of the Royal Astronomical Society. 2018 ; Vol. 476, No. 1. pp. 520-527.
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abstract = "We report on the astrometric registration of very long baseline interferometry images of the SiO and H2O masers in OH231.8+4.2, the iconic proto-planetary nebula also known as the Calabash nebula, using the Korean VLBI Network and source frequency phase referencing. This, for the first time, robustly confirms the alignment of the SiO masers, close to the asymptotic giant branch star, driving the bilobe structure with the water masers in the outflow. We are able to trace the bulk motions for the H2O masers over the last few decades to be 19 km s-1 and deduce that the age of this expansion stage is 38±2 yr. The combination of this result with the distance allows a full 3D reconstruction and confirms that the H2O masers lie on and expand along the known large-scale symmetry axis and that the outflow is only a few decades old, so mass loss is almost certainly ongoing. Therefore, we conclude that the SiO emission marks the stellar core of the nebular, the H2O emission traces the expansion, and there must be multiple epochs of ejection to drive the macro-scale structure.",
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Registration of H2O and SiO masers in the Calabash Nebula to confirm the planetary nebula paradigm. / Dodson, R.; Rioja, M.; Bujarrabal, V.; Kim, J.; Cho, S. H.; Choix, Y. K.; Youngjoo, Y.

In: Monthly Notices of the Royal Astronomical Society, Vol. 476, No. 1, 01.05.2018, p. 520-527.

Research output: Contribution to journalArticle

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AU - Rioja, M.

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AU - Cho, S. H.

AU - Choix, Y. K.

AU - Youngjoo, Y.

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