Amanote Research

Amanote Research

    RegisterSign In

Estimates of Stellar Weak Interaction Rates for Nuclei in the Mass RangeA = 65–80

Astrophysical Journal, Supplement Series - United States
doi 10.1086/376753
Full Text
Open PDF
Abstract

Available in full text

Categories
AstrophysicsAstronomyPlanetary ScienceSpace
Date

November 1, 2003

Authors
Jason PruetGeorge M. Fuller
Publisher

IOP Publishing


Related search

Revised Rates of Stellar Disruption in Galactic Nuclei

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2004English

The Stellar Content of Elliptical Nuclei

Highlights of Astronomy
1983English

Stellar Winds and Mass-Loss Rates From Be Stars

Symposium - International Astronomical Union
1982English

The Effect of Distant Large Scale Structure on Weak Lensing Mass Estimates

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2001English

A New Method to Measure Stellar Mass-Loss Rates

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2009English

Non-Axial Octupole Deformations of N=Z Nuclei in A∼60–80 Mass Region

1999English

Stellar Population in the Nuclei of Early–type Galaxies

Symposium - International Astronomical Union
1993English

Consistent Approach to Weak Interaction Rates Based on the Relativistic QRPA

2009English

Revisited Mass-Loss Rates of Planetary Nebula Nuclei Observed With IUE

Symposium - International Astronomical Union
1989English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy