Post-common envelope PN, fundamental or irrelevant?

Orsola De Marco; T. Reichardt; R. Iaconi; T. Hillwig; G. H. Jacoby; D. Keller; R. G. Izzard; J. Nordhaus; E. G. Blackman

doi:10.1017/S1743921317002149

Post-common envelope PN, fundamental or irrelevant?

Orsola De Marco, T. Reichardt, R. Iaconi, T. Hillwig, G. H. Jacoby, D. Keller, R. G. Izzard, J. Nordhaus, E. G. Blackman

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

1 Citation (Scopus)

Abstract

One in 5 PN are ejected from common envelope binary interactions but Kepler results are already showing this proportion to be larger. Their properties, such as abundances can be starkly different from those of the general population, so they should be considered separately when using PN as chemical or population probes. Unfortunately post-common envelope PN cannot be discerned using only their morphologies, but this will change once we couple our new common envelope simulations with PN formation models.

Original language	English
Title of host publication	Planetary nebulae : multi-wavelength probes of stellar and galactic evolution
Subtitle of host publication	proceedings of the 323rd symposium of the International Astronomical Union held in Beijing, China October 10-14, 2016
Editors	Xiaowei Liu, Letizia Stanghellini, Amanda Karakas
Place of Publication	Cambridge
Publisher	Cambridge University Press (CUP)
Pages	213-217
Number of pages	5
ISBN (Print)	9781107169913
DOIs	https://doi.org/10.1017/S1743921317002149
Publication status	Published - 2017
Event	323rd symposium of the International Astronomical Union - Beijing, China Duration: 10 Oct 2016 → 14 Oct 2016

Publication series

Name	IAU symposium
Publisher	Cambridge University Press
Number	323
ISSN (Print)	1743-9213

Conference

Conference	323rd symposium of the International Astronomical Union
Country	China
City	Beijing
Period	10/10/16 → 14/10/16

Keywords

binaries (including multiple): close
hydrodynamics
planetary nebulae: general
stars: AGB and post-AGB
stars: evolution
stars: statistics

Access to Document

10.1017/S1743921317002149

Link to publication in Scopus

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De Marco, O., Reichardt, T., Iaconi, R., Hillwig, T., Jacoby, G. H., Keller, D., Izzard, R. G., Nordhaus, J., & Blackman, E. G. (2017). Post-common envelope PN, fundamental or irrelevant? In X. Liu, L. Stanghellini, & A. Karakas (Eds.), Planetary nebulae : multi-wavelength probes of stellar and galactic evolution: proceedings of the 323rd symposium of the International Astronomical Union held in Beijing, China October 10-14, 2016 (pp. 213-217). (IAU symposium; No. 323). Cambridge University Press (CUP). https://doi.org/10.1017/S1743921317002149

De Marco, Orsola ; Reichardt, T. ; Iaconi, R. ; Hillwig, T. ; Jacoby, G. H. ; Keller, D. ; Izzard, R. G. ; Nordhaus, J. ; Blackman, E. G. / Post-common envelope PN, fundamental or irrelevant?. Planetary nebulae : multi-wavelength probes of stellar and galactic evolution: proceedings of the 323rd symposium of the International Astronomical Union held in Beijing, China October 10-14, 2016. editor / Xiaowei Liu ; Letizia Stanghellini ; Amanda Karakas. Cambridge : Cambridge University Press (CUP), 2017. pp. 213-217 (IAU symposium; 323).

@inproceedings{39ef8c8c95a1455da0f8f5371e355fa9,

title = "Post-common envelope PN, fundamental or irrelevant?",

abstract = "One in 5 PN are ejected from common envelope binary interactions but Kepler results are already showing this proportion to be larger. Their properties, such as abundances can be starkly different from those of the general population, so they should be considered separately when using PN as chemical or population probes. Unfortunately post-common envelope PN cannot be discerned using only their morphologies, but this will change once we couple our new common envelope simulations with PN formation models.",

keywords = "binaries (including multiple): close, hydrodynamics, planetary nebulae: general, stars: AGB and post-AGB, stars: evolution, stars: statistics",

author = "{De Marco}, Orsola and T. Reichardt and R. Iaconi and T. Hillwig and Jacoby, {G. H.} and D. Keller and Izzard, {R. G.} and J. Nordhaus and Blackman, {E. G.}",

year = "2017",

doi = "10.1017/S1743921317002149",

language = "English",

isbn = "9781107169913",

series = "IAU symposium",

publisher = "Cambridge University Press (CUP)",

number = "323",

pages = "213--217",

editor = "Xiaowei Liu and Letizia Stanghellini and Amanda Karakas",

booktitle = "Planetary nebulae : multi-wavelength probes of stellar and galactic evolution",

note = "323rd symposium of the International Astronomical Union ; Conference date: 10-10-2016 Through 14-10-2016",

}

De Marco, O, Reichardt, T, Iaconi, R, Hillwig, T, Jacoby, GH, Keller, D, Izzard, RG, Nordhaus, J & Blackman, EG 2017, Post-common envelope PN, fundamental or irrelevant? in X Liu, L Stanghellini & A Karakas (eds), Planetary nebulae : multi-wavelength probes of stellar and galactic evolution: proceedings of the 323rd symposium of the International Astronomical Union held in Beijing, China October 10-14, 2016. IAU symposium, no. 323, Cambridge University Press (CUP), Cambridge, pp. 213-217, 323rd symposium of the International Astronomical Union, Beijing, China, 10/10/16. https://doi.org/10.1017/S1743921317002149

Post-common envelope PN, fundamental or irrelevant? / De Marco, Orsola; Reichardt, T.; Iaconi, R.; Hillwig, T.; Jacoby, G. H.; Keller, D.; Izzard, R. G.; Nordhaus, J.; Blackman, E. G.

Planetary nebulae : multi-wavelength probes of stellar and galactic evolution: proceedings of the 323rd symposium of the International Astronomical Union held in Beijing, China October 10-14, 2016. ed. / Xiaowei Liu; Letizia Stanghellini; Amanda Karakas. Cambridge : Cambridge University Press (CUP), 2017. p. 213-217 (IAU symposium; No. 323).

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