• The German eROSITA Consortium (eROSITA-DE) makes public the first six months of the SRG/eROSITA all-sky ...
    while data with 359.94423568 > l >179.94423568 degrees (Western Galactic hemisphere) belong to eROSITA-DE ...
    equator to more than 10,000 seconds close to the Ecliptic pole in the 0.6—2.3 keV energy band. eROSITA-DE ...
    For a more detailed description of the data types, please refer to eROSITA-DE:DataRelease1:eSASS4DR1_ ...
  • 北京大学博士生孙唯佳、段晓苇与国家天文台邓李才研究员、澳大利亚麦考瑞大学Richard de Grijs教授、北京师范大学博士后章博、国家天文台刘超研究员合作,基于LAMOST中分辨率光谱,构建了目前最大样本的早型星星表 ...
    早型星是一类光谱类型为O、B、A或早F、温度高、质量大的明亮恒星。与质量较小的晚型矮星相比,它们的寿命较短,数量较少。
  • 在LAMOST-Kepler项目低分辨率光谱巡天取得重要进展和系列成果(De Cat et al. 2015, Zong et al. 2018,Fu et al. 2020)的基础上,随着LAMOST ...
    -N., De Cat, P., et al. 2020, ApJS, 251, 16 Fu, J.
    ., De Cat, P., Zong, W., et al. 2020, RAA, 20, 167 Liu, N., Fu, J.
    -N., De Cat, P., et al. 2018, ApJS, 238, 30 De Cat, P., Fu, J.-N., Ren, A.
  • Any proposals that do not list the current status of previous allocations to investigators will be penalized ...
    Do not exceed the page limits, or put information in the wrong sections of the proposal in order to circumvent ...
  •   – Jose Maza, Education of Astronomy in all levels (Universidad de Chile, Chile).
    of women in Astronomy in promoting education and culture   (Observatorio Nacional Coordenação ...
    de Pesquisas em Astronomia e Astrofisica, Brazil)           此外,在本次会议闭幕式上,所有与会人员还将共同欣赏 ...
  • 更多详情,请访问https://sites.google.com/cfa.harvard.edu/saoimageds9/about 图2 DS9界面 奖项将在2024年ADASS会议期间颁发, ...
  • sources in the roughly following range: −0.5 < BP − RP < 2 3 < G < 17.5  E(B − V) < 0.8 Sources that do ...
  • sources in the roughly following range: −0.5 < BP − RP < 2 3 < G < 17.5  E(B − V) < 0.8 Sources that do ...
  • “Models show that our current theories about how stars evolve do not predict this Lithium production ...
  • Ministry for Higher Education Research and Innovation, MESRI)、法国国家科学研究中心国家地球科学和天文研究所(Centre national de ...
    la recherche scientifique - Institut national des sciences de l'Univers,CNRS-INSU)、斯特拉斯堡大学、法国国家科学中心开放研究数据部门 ...
  • 德国 eROSITA 联盟 (eROSITA-DE) 于2024年1月31日公开了 SRG/eROSITA 全天巡天调查 (eRASS1) 前六个月的数据,这些数据的专有权属于德国 eROSITA联盟。
    eROSITA-DE DR1公开了 0.2—10 千电子伏特能量频段的校准事件列表、图像、曝光图、背景图和灵敏度图,以及不同能量频段的流量上限。此外,还发布了选定(明亮)目标的源光谱和光变曲线。
    关于数据类型更详细的描述可参考 https://erosita.mpe.mpg.de/dr1/eSASS4DR1/eSASS4DR1_ProductsDescription/products_description_dr1 ...
  • | ...
  • Much like the catalogs such as UCAC or GAIA do for astrometry, APASS gives the ability to photometrically ...
  • Bulletin de la Société Royale des Sciences de Liège, Vol. 87, Actes de colloques ...
  • 近日,国家天文台李广伟副研究员在LAMOST光谱数据中筛选出209颗O型星,其中135颗是最新发现的。这是迄今为止利用单一光谱数据库,一次性新发现银河系O型星数量最多的研究工作。
    在这之前,最大的具有光谱信息的银河系O型星星表(Galactic O-Star Catalog; GOSC),仅有590颗O型星,且这些O型星是人类近百年来累积发现的总和。
    ,这就导致了我们很难找到大质量的O型星。
    星,将会增进人们对O型星的星风和星周物质的盘等理论研究有重要意义;该成果中还包含一些较暗的,处于银河系外旋臂的O型星。
    另外,把LAMOST发现的O型星与前人公布的光谱数据比较,还发现了一些呈现光谱变化的O型星。
  • 不同的强线指标(Ne₃O₂和O₃₂)得到的电离气体的电离度也比较一致(尤其是在高电离度区间),而且没有明显的红移演化。
    图2 强[O III]λ5007发射线致密星系N/O和金属丰度的关系。
    在低金属丰度的区间,强[O III]λ5007发射线的致密星系中氮和氧的比例(N/O)关系偏高(见图2),其中的氮元素主要来自初级核合成,研究团队认为强发射线致密星系的氮元素增丰很可能是星系周围气体内流导致的 ...
    图3 八个具有不对称[O III]λ5007发射线结构的光谱轮廓。
    研究团队通过对强[O III]λ5007发射线致密星系的金属丰度和发射线轮廓进行分析,发现位于离散环境中的强[O III]λ5007发射线致密星系在很大程度上可能是受到星系周围气体内流和外流的影响 ...
  • This article reports a sample of 1830 strong [O iii]λ5007 emission-line compact galaxies discovered with ...
    We newly identify 402 spectra of 346 strong [O iii]λ5007 emission-line compact galaxies by finding compact ...
    The N/O measurements of the strong [O iii]λ5007 emission-line compact galaxies mainly locate at a plateau ...
    The Ne3O2 and O32 relation follows a tight linear relation with no redshift evolution.
    The Ne3O2 anti-correlates with the stellar mass, and at fixed stellar mass the Ne3O2 increase with the ...
  • This article reports a sample of 1830 strong [O iii]λ5007 emission-line compact galaxies discovered with ...
    We newly identify 402 spectra of 346 strong [O iii]λ5007 emission-line compact galaxies by finding compact ...
    The N/O measurements of the strong [O iii]λ5007 emission-line compact galaxies mainly locate at a plateau ...
    The Ne3O2 and O32 relation follows a tight linear relation with no redshift evolution.
    The Ne3O2 anti-correlates with the stellar mass, and at fixed stellar mass the Ne3O2 increase with the ...
  • This article reports a sample of 1830 strong [O iii]λ5007 emission-line compact galaxies discovered with ...
    We newly identify 402 spectra of 346 strong [O iii]λ5007 emission-line compact galaxies by finding compact ...
    The N/O measurements of the strong [O iii]λ5007 emission-line compact galaxies mainly locate at a plateau ...
    The Ne3O2 and O32 relation follows a tight linear relation with no redshift evolution.
    The Ne3O2 anti-correlates with the stellar mass, and at fixed stellar mass the Ne3O2 increase with the ...
  • This article reports a sample of 1830 strong [O iii]λ5007 emission-line compact galaxies discovered with ...
    We newly identify 402 spectra of 346 strong [O iii]λ5007 emission-line compact galaxies by finding compact ...
    The N/O measurements of the strong [O iii]λ5007 emission-line compact galaxies mainly locate at a plateau ...
    The Ne3O2 and O32 relation follows a tight linear relation with no redshift evolution.
    The Ne3O2 anti-correlates with the stellar mass, and at fixed stellar mass the Ne3O2 increase with the ...
  •  
我们使用cookies为您提供更好的体验。继续使用本网站,即表示您同意按照我们的Cookie 政策使用cookie。
接受