Free shipping on orders over $99
Surface Inhomogeneities on Late-Type Stars

Surface Inhomogeneities on Late-Type Stars

Proceedings of a Colloquium Held at Armagh Observatory, Northern Ireland, 24-27 July 1990

by Patrick B. Byrne and Dermott J. Mullan
Paperback
Publication Date: 12/09/2014

Share This Book:

  $169.00
or 4 easy payments of $42.25 with
afterpay
This item qualifies your order for FREE DELIVERY
The contributions in this volume discuss the magnetic structures in the outer atmospheres of active late-type stars, and in particular the various methods available for imaging surface features on these objects. Emphasis has been laid upon multiwavelength studies of the phenomena and the application of solar astrophysics to stellar objects. The book is recommended to research workers or postgraduate students in stellar astrophysics.
ISBN:
9783662138847
9783662138847
Category:
Astrophysics
Format:
Paperback
Publication Date:
12-09-2014
Language:
English
Publisher:
Springer
Country of origin:
United States
Dimensions (mm):
244x170mm
Weight:
0.65kg

This title is in stock with our Australian supplier and should arrive at our Sydney warehouse within 2 - 3 weeks of you placing an order.

Once received into our warehouse we will despatch it to you with a Shipping Notification which includes online tracking.

Please check the estimated delivery times below for your region, for after your order is despatched from our warehouse:

ACT Metro: 2 working days
NSW Metro: 2 working days
NSW Rural: 2-3 working days
NSW Remote: 2-5 working days
NT Metro: 3-6 working days
NT Remote: 4-10 working days
QLD Metro: 2-4 working days
QLD Rural: 2-5 working days
QLD Remote: 2-7 working days
SA Metro: 2-5 working days
SA Rural: 3-6 working days
SA Remote: 3-7 working days
TAS Metro: 3-6 working days
TAS Rural: 3-6 working days
VIC Metro: 2-3 working days
VIC Rural: 2-4 working days
VIC Remote: 2-5 working days
WA Metro: 3-6 working days
WA Rural: 4-8 working days
WA Remote: 4-12 working days

Reviews

Be the first to review Surface Inhomogeneities on Late-Type Stars.