找回密碼
 To register

QQ登錄

只需一步,快速開(kāi)始

掃一掃,訪問(wèn)微社區(qū)

打印 上一主題 下一主題

Titlebook: Comets to Cosmology; Proceedings of the T Andrew Lawrence Conference proceedings 1988 Springer-Verlag Berlin Heidelberg 1988 Redshift.aster

[復(fù)制鏈接]
樓主: corrode
51#
發(fā)表于 2025-3-30 11:35:25 | 只看該作者
Christian Seelos,Kate Ganly,Johanna Mairnd albedo of ~0.05. It is inferred that the nucleus itself is dark. Upper limits on the number density of trail particles are calulated. The mean free path between trail particles suggests that the Comet Rendevous/Asteroid Flyby mission is unlikely to be affected if it flies within the trail ahead o
52#
發(fā)表于 2025-3-30 16:00:24 | 只看該作者
Social Enterprise Theoretical Framework,a physical model that describes at the four IRAS wavelengths the contaminating contribution of the zodiacal emission. Direct comparison between the 100 . and HI column density maps shows a good correlation at high galactic latitudes. After radial unfolding the 12, 25, 60 and 100 . radial profiles ar
53#
發(fā)表于 2025-3-30 19:06:11 | 只看該作者
https://doi.org/10.1007/978-3-319-01396-1 used as a very rigid observational constraint of the model. It is found that dust associated with atomic hydrogen is the dominant contribution to the total infrared luminosity. Correlations between warm and cold dust emission. HII regions and the distribution of the atomic gas are analyzed. Dust pr
54#
發(fā)表于 2025-3-30 23:57:17 | 只看該作者
55#
發(fā)表于 2025-3-31 03:00:51 | 只看該作者
56#
發(fā)表于 2025-3-31 06:47:58 | 只看該作者
The Challenge of Public Goods Provisionhe origin of the infrared emission from the solar neigbourhood. We show that altough most of the emission comes from interstellar matter not associated with current star formation, about half of the heating of grains is provided by ultraviolet photons radiated by stars younger than few 10. yrs.
57#
發(fā)表于 2025-3-31 11:30:18 | 只看該作者
58#
發(fā)表于 2025-3-31 13:55:08 | 只看該作者
59#
發(fā)表于 2025-3-31 18:51:05 | 只看該作者
60#
發(fā)表于 2025-4-1 01:34:16 | 只看該作者
https://doi.org/10.1007/BFb0118781Redshift; asteroid; astronomy; cosmic microwave background; cosmology; solar system; star; star formation
 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(ài)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.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國(guó)際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-17 13:44
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
秦安县| 东乌| 井研县| 尼木县| 察雅县| 福泉市| 静乐县| 历史| 慈利县| 板桥市| 开封市| 府谷县| 农安县| 双峰县| 普安县| 绥德县| 高安市| 达州市| 林甸县| 阿克陶县| 河北省| 雷山县| 肥东县| 岱山县| 锡林郭勒盟| 客服| 应用必备| 禄丰县| 重庆市| 三原县| 铜川市| 柳江县| 乳山市| 泾阳县| 元氏县| 克什克腾旗| 西峡县| 武胜县| 东方市| 娄底市| 舞钢市|