Kinematics and dynamics of the Galactic bulge through planetary nebulae

A. E J Peyaud; C. Boily; A. Acker; Q. Parker

doi:10.1017/S1743921306003863

Kinematics and dynamics of the Galactic bulge through planetary nebulae

A. E J Peyaud^*, C. Boily, A. Acker, Q. Parker

^*Corresponding author for this work

Research output: Contribution to journal › Article

Abstract

The discovery of ∼500 planetary nebulae (PNe) in the bulge region allows us to probe the bulge out to ∼ 8 kpc. This opens up the possibility to track bulge-disc interactions to unprecedented details. We present an exploration of bulge dynamics with Nbody models of a triaxial bulge embedded in an exponential disc (Peyaud 2005).

Original language	English
Pages (from-to)	485-486
Number of pages	2
Journal	Proceedings of the International Astronomical Union
Volume	2
Issue number	234
DOIs	https://doi.org/10.1017/S1743921306003863
Publication status	Published - Apr 2006

Keywords

Dynamics
Kinematics
Planetary nebulae

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10.1017/S1743921306003863

Cite this

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title = "Kinematics and dynamics of the Galactic bulge through planetary nebulae",

abstract = "The discovery of ∼500 planetary nebulae (PNe) in the bulge region allows us to probe the bulge out to ∼ 8 kpc. This opens up the possibility to track bulge-disc interactions to unprecedented details. We present an exploration of bulge dynamics with Nbody models of a triaxial bulge embedded in an exponential disc (Peyaud 2005).",

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author = "Peyaud, {A. E J} and C. Boily and A. Acker and Q. Parker",

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language = "English",

volume = "2",

pages = "485--486",

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AU - Peyaud, A. E J

AU - Boily, C.

AU - Acker, A.

AU - Parker, Q.

PY - 2006/4

Y1 - 2006/4

N2 - The discovery of ∼500 planetary nebulae (PNe) in the bulge region allows us to probe the bulge out to ∼ 8 kpc. This opens up the possibility to track bulge-disc interactions to unprecedented details. We present an exploration of bulge dynamics with Nbody models of a triaxial bulge embedded in an exponential disc (Peyaud 2005).

AB - The discovery of ∼500 planetary nebulae (PNe) in the bulge region allows us to probe the bulge out to ∼ 8 kpc. This opens up the possibility to track bulge-disc interactions to unprecedented details. We present an exploration of bulge dynamics with Nbody models of a triaxial bulge embedded in an exponential disc (Peyaud 2005).

KW - Dynamics

KW - Kinematics

KW - Planetary nebulae

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U2 - 10.1017/S1743921306003863

DO - 10.1017/S1743921306003863

M3 - Article

AN - SCOPUS:33845533791

VL - 2

SP - 485

EP - 486

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - 234

ER -

Kinematics and dynamics of the Galactic bulge through planetary nebulae

Abstract

Keywords

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