Titlebook: Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites; Proceedings of the E Sofia Randich,Luca Pasquini Conference pr

只看該作者 · 發(fā)表于 2025-3-30 11:04:00

FOR XML and Legacy XML Support,ially for those stars presenting a misclassification from the evolutionary tracks. Our stars sample presents three giants with extra solar planets detection HD 47536, HD 122430 and HD 11977 (Figure 1). In addition, derived CNO abundances permit to study the behavior of these elements in low mass (M

只看該作者 · 發(fā)表于 2025-3-30 14:50:51

CNO Abundances in Giants with Precise Radial Velocity Measurementsially for those stars presenting a misclassification from the evolutionary tracks. Our stars sample presents three giants with extra solar planets detection HD 47536, HD 122430 and HD 11977 (Figure 1). In addition, derived CNO abundances permit to study the behavior of these elements in low mass (M

只看該作者 · 發(fā)表于 2025-3-30 16:46:01

只看該作者 · 發(fā)表于 2025-3-31 00:30:52

只看該作者 · 發(fā)表于 2025-3-31 04:03:16

只看該作者 · 發(fā)表于 2025-3-31 06:56:14

只看該作者 · 發(fā)表于 2025-3-31 12:38:31

只看該作者 · 發(fā)表于 2025-3-31 14:55:01

只看該作者 · 發(fā)表于 2025-3-31 17:43:40

		自動(dòng)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(diǎn)評(píng)	投稿經(jīng)驗(yàn)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, 2025-10-11 18:55
Copyright © 2001-2015 派博傳思京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved