主要内容:
整体上有统计关系,但是各个类别内部并不按照总的来。
精彩摘抄:
 |
有这么多数据 |
 |
总的关系 |
文章信息:
- · Full Refereed Journal Article (PDF/Postscript)
- · Full Refereed Scanned Article (GIF)
- · References in the article
- · Citations to the Article (14) (Citation History)
- · Refereed Citations to the Article
- · SIMBAD Objects (4)
- · Also-Read Articles (Reads History)
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Title: |
| Magnetic moments and angular momenta of stars and planets |
Authors: |
| Arge, C. N.; Mullan, D. J.; Dolginov, A. Z. |
Affiliation: |
| AA(University of Delaware, Newark, DE, US), AB(University of Delaware, Newark, DE, US), AC(Lunar and Planetary Institute, Houston, TX, US) |
Publication: |
| Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 443, no. 2, p. 795-803 (ApJ Homepage) |
Publication Date: |
| 04/1995 |
Category: |
| Astrophysics |
Origin: |
| STI |
NASA/STI Keywords: |
| ANGULAR MOMENTUM, CORRELATION, DATA BASES, MAGNETIC MOMENTS, PLANETS, STARS, CENTER OF GRAVITY, LOGARITHMS, MAGNETIC FIELDS, MASS, RADII, ROTATION, SOLAR SYSTEM |
DOI: |
| 10.1086/175569 |
Bibliographic Code: |
| 1995ApJ...443..795A |
Abstract
Using published data on magnetic fields, radii, masses, and rotation, we have compiled a data set of magnetic moments mu and angular momenta L for stars and planets. In our subsample of hotter stars (classes A, B, and O), there are 171 objects. In the subsample of cooler stars (classes F, G, K, and M), there are 54 objects. We include 33 white dwarfs, of which 19 are in cataclysmic variables. The pulsar subsample contains 32 pulsars in binaries and 429 isolated pulsars. Som subsamples exhibit significant empirical correlations between log mu and log L. For the hot and cool stars, the correlations are positive. However, the hot-star correlation is significantly shallower than for the cool stars. In the solar system subsample, the correlation has essentially the same slope as for the cool stars, although the magnetic moments are two to three orders of magnitude smaller for the solar system objects at a given L value. For isolated white dwarfs, the correlations are weak or absent. Pulsars and white dwarfs in close binaries show strong negative correlations: the results are quantitatively consistent with magnetically enforced synchronism with the orbital period. When we consider the centers of gravity of the different subsamples of objects, a significant positive correlation appears between log mu and log L.
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