Amanote Research

Amanote Research

    RegisterSign In

A Triaxial Model for the Bulge of NGC 4697

Symposium - International Astronomical Union
doi 10.1017/s007418090012399x
Full Text
Open PDF
Abstract

Available in full text

Date

January 1, 1993

Authors
W.W. ZeilingerM.L. WinsallH. Dejonghe
Publisher

Cambridge University Press (CUP)


Related search

Kinematic Evidence for Different Planetary Nebulae Populations in the Elliptical Galaxy NGC 4697

AIP Conference Proceedings
AstronomyPhysics
2005English

SOARBVIphotometry of the Metal-Poor Bulge Globular Cluster NGC 6642

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

Chemical Analysis of NGC 6528: One of the Most Metal-Rich Bulge Globular Clusters

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2018English

Triaxial Composite Model for Basic Creep of Concrete

Journal of Engineering Mechanics - ASCE
Mechanics of MaterialsMechanical Engineering
1998English

A Two-Phase Model for the Narrow Line Region of NGC 4151

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2001English

Bulge and Disk: A Simple Self-Gravitating Model

Symposium - International Astronomical Union
1993English

A 3D Kinematic Model of NGC 3242

Symposium - International Astronomical Union
1997English

A Photoionization Model Study of NGC 7027

Symposium - International Astronomical Union
1989English

Kinematical Features of the Main Bulge in a Multi-Component Galactic Model

Symposium - International Astronomical Union
1993English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2026 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy