Titlebook: Radio Stars; Proceedings of a Wor Robert M. Hjellming,David M. Gibson Conference proceedings 1985 D. Reidel Publishing Company, Dordrecht,

只看該作者 · 發(fā)表于 2025-3-31 11:18:18

Synchrotron Emission from Chaotic Stellar Windsmodel can account for many of the observed characteristics of some recently discovered stars which have peculiar radio emission. The magnetic fields which are required are quite small (1 to 10 Gauss at the surface of the star). High energy particles accelerated by shocks near the star may also make hot stars significant sources of γ-rays.

只看該作者 · 發(fā)表于 2025-3-31 15:37:44

只看該作者 · 發(fā)表于 2025-3-31 18:23:27

只看該作者 · 發(fā)表于 2025-4-1 01:25:24

		自動登錄	找回密碼
密碼			To register

關(guān)于派博傳思			派博傳思旗下網(wǎng)站			友情鏈接
派博傳思介紹	公司地理位置	論文服務(wù)流程	影響因子官網(wǎng)	吾愛論文網(wǎng)	大講堂	北京大學(xué)	Oxford Uni.	Harvard Uni.
發(fā)展歷史沿革	期刊點評	投稿經(jīng)驗總結(jié)	SCIENCEGARD	IMPACTFACTOR	派博系數(shù)	清華大學(xué)	Yale Uni.	Stanford Uni.
\|Archiver\|手機(jī)版\|小黑屋\| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-10 01:25
Copyright © 2001-2015 派博傳思京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved