A detailed spatiokinematic model of the multipolar planetary nebula NGC 7026

被引：1

作者：

Clark, David M. ^{[1
]}

Alberto Lopez, Jose ^{[1
]}

Steffen, Wolfgang ^{[1
]}

Richer, Michael G. ^{[1
]}

机构：

[1] Univ Nacl Autonoma Mexico, Inst Astron, Ensenada 22800, Baja California, Mexico

来源：

PLANETARY NEBULAE: AN EYE TO THE FUTURE | 2012年 / 283期

关键词：

ISM: kinematics and dynamics; planetary nebulae: general; planetary nebulae: individual (NGC 7026); SHAPE;

D O I：

10.1017/S1743921312011283

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the most extensive, long-slit, high-resolution coverage of the complex planetary nebula (PN), NGC 7026. Ten spectra were acquired using the Manchester Echelle Spectrometer at San Pedro Martir Observatory in Baja California, Mexico, and each shows exquisite detail, revealing the intricate structure of this object. Incorporating these spectra into the 3-dimensional visualization and kinematic program, Shape, and using HST images of NGC 7026, we have produced a detailed structural and kinematic model of this PN. Knowledge of the 3-D structure of this nebula is relevant to understand the physics behind the extended X-ray emission in this object.

引用

页码：332 / 333

页数：2

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