Titlebook: Cataclysmic Variables and Low-Mass X-Ray Binaries; Proceedings of the 7 Donald Q. Lamb,Joseph Patterson Conference proceedings 1985 D. Reid

只看該作者 · 發(fā)表于 2025-3-27 00:25:03

The Mass Transfer Rate in X1916-053: Is it Driven by Gravitational Radiation?xpected from gravitational radiation (GR). Within uncertainty of a factor of 2 the transfer rate for the composite model solution is consistent with GR, but enhancement by other mechanisms should be investigated.

只看該作者 · 發(fā)表于 2025-3-27 03:52:22

只看該作者 · 發(fā)表于 2025-3-27 06:42:25

只看該作者 · 發(fā)表于 2025-3-27 12:38:07

只看該作者 · 發(fā)表于 2025-3-27 13:48:09

只看該作者 · 發(fā)表于 2025-3-27 19:29:57

只看該作者 · 發(fā)表于 2025-3-27 22:38:18

Alister Miskimmon,Ben O’Loughlinects, is presented. The resulting appearance is compared to recent observations of X-ray dips in several X-ray binaries. We also discuss the dynamical effects of X-ray induced mass loss, which originates at large radius in the disk.

只看該作者 · 發(fā)表于 2025-3-28 02:38:54

只看該作者 · 發(fā)表于 2025-3-28 09:00:40

只看該作者 · 發(fā)表于 2025-3-28 12:50:25

		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, 2025-10-6 05:31
Copyright © 2001-2015 派博傳思京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved