Post-AGB stars in the LMC and SMC

Hans Van Winckel; Els Van Aarle; Peter R. Wood; Devika Kamath; Tom Lloyd Evans; Kenneth De Smedt; Nadya Gorlova; Clio Gielen

doi:10.1017/S1743921312011015

Post-AGB stars in the LMC and SMC

Hans Van Winckel^*, Els Van Aarle, Peter R. Wood, Devika Kamath, Tom Lloyd Evans, Kenneth De Smedt, Nadya Gorlova, Clio Gielen

^*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

Galactic post-AGB stars show a large diversity in chemical compositions as well as in the kinematical and geometrical properties of their circumstellar material. The theoretical interpretation is hampered by the lack of good distances to almost all Galactic objects. We therefore initiated a large project to study systematically post-AGB stars in the Large and Small Magellanic Cloud (LMC, SMC respectively). Here we report on our preliminary results.

Original language	English
Title of host publication	Planetary Nebulae
Subtitle of host publication	An Eye to the Future
Editors	Arturo Manchado, Letizia Stanghellini, Detlef Schonberner
Pages	235-238
Number of pages	4
Edition	S283
DOIs	https://doi.org/10.1017/S1743921312011015
Publication status	Published - Jul 2011

Publication series

Name	Proceedings of the International Astronomical Union
Number	S283
Volume	7
ISSN (Print)	1743-9213
ISSN (Electronic)	1743-9221

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10.1017/S1743921312011015

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Van Winckel, H., Van Aarle, E., Wood, P. R., Kamath, D., Evans, T. L., De Smedt, K., Gorlova, N., & Gielen, C. (2011). Post-AGB stars in the LMC and SMC. In A. Manchado, L. Stanghellini, & D. Schonberner (Eds.), Planetary Nebulae: An Eye to the Future (S283 ed., pp. 235-238). (Proceedings of the International Astronomical Union; Vol. 7, No. S283). https://doi.org/10.1017/S1743921312011015

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title = "Post-AGB stars in the LMC and SMC",

abstract = "Galactic post-AGB stars show a large diversity in chemical compositions as well as in the kinematical and geometrical properties of their circumstellar material. The theoretical interpretation is hampered by the lack of good distances to almost all Galactic objects. We therefore initiated a large project to study systematically post-AGB stars in the Large and Small Magellanic Cloud (LMC, SMC respectively). Here we report on our preliminary results.",

keywords = "Magellanic Clouds, Stars: AGB and post-AGB, circumstellar matter, stars: evolution",

author = "{Van Winckel}, Hans and {Van Aarle}, Els and Wood, {Peter R.} and Devika Kamath and Evans, {Tom Lloyd} and {De Smedt}, Kenneth and Nadya Gorlova and Clio Gielen",

year = "2011",

month = jul,

doi = "10.1017/S1743921312011015",

language = "English",

isbn = "9781107019836",

series = "Proceedings of the International Astronomical Union",

number = "S283",

pages = "235--238",

editor = "Arturo Manchado and Letizia Stanghellini and Detlef Schonberner",

booktitle = "Planetary Nebulae",

edition = "S283",

}

Post-AGB stars in the LMC and SMC. / Van Winckel, Hans; Van Aarle, Els; Wood, Peter R. et al.
Planetary Nebulae: An Eye to the Future. ed. / Arturo Manchado; Letizia Stanghellini; Detlef Schonberner. S283. ed. 2011. p. 235-238 (Proceedings of the International Astronomical Union; Vol. 7, No. S283).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - Post-AGB stars in the LMC and SMC

AU - Van Winckel, Hans

AU - Van Aarle, Els

AU - Wood, Peter R.

AU - Kamath, Devika

AU - Evans, Tom Lloyd

AU - De Smedt, Kenneth

AU - Gorlova, Nadya

AU - Gielen, Clio

PY - 2011/7

Y1 - 2011/7

N2 - Galactic post-AGB stars show a large diversity in chemical compositions as well as in the kinematical and geometrical properties of their circumstellar material. The theoretical interpretation is hampered by the lack of good distances to almost all Galactic objects. We therefore initiated a large project to study systematically post-AGB stars in the Large and Small Magellanic Cloud (LMC, SMC respectively). Here we report on our preliminary results.

AB - Galactic post-AGB stars show a large diversity in chemical compositions as well as in the kinematical and geometrical properties of their circumstellar material. The theoretical interpretation is hampered by the lack of good distances to almost all Galactic objects. We therefore initiated a large project to study systematically post-AGB stars in the Large and Small Magellanic Cloud (LMC, SMC respectively). Here we report on our preliminary results.

KW - Magellanic Clouds

KW - Stars: AGB and post-AGB

KW - circumstellar matter

KW - stars: evolution

UR - http://www.scopus.com/inward/record.url?scp=84865746295&partnerID=8YFLogxK

U2 - 10.1017/S1743921312011015

DO - 10.1017/S1743921312011015

M3 - Conference contribution

SN - 9781107019836

T3 - Proceedings of the International Astronomical Union

SP - 235

EP - 238

BT - Planetary Nebulae

A2 - Manchado, Arturo

A2 - Stanghellini, Letizia

A2 - Schonberner, Detlef

ER -

Post-AGB stars in the LMC and SMC

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