天文研究与技术-国家天文台台刊
天文研究與技術-國傢天文檯檯刊
천문연구여기술-국가천문태태간
ASTRONOMICAL RESEARCH & TECHNOLOGY-PUBLICATIONS OF NATIONAL ASTRONOMICAL OBSERVATORIES OF CHINA
2005年
4期
209-217
,共9页
谢照华%张雄%刘洪涛%杜雷鸣
謝照華%張雄%劉洪濤%杜雷鳴
사조화%장웅%류홍도%두뢰명
活动星系核%伽玛射线噪-宇宙学%观测-宇宙学%红移-哈勃图
活動星繫覈%伽瑪射線譟-宇宙學%觀測-宇宙學%紅移-哈勃圖
활동성계핵%가마사선조-우주학%관측-우주학%홍이-합발도
AGN:Gamma-ray-loud-cosmology%observation-cosmology%redshift-Hubble diagrarn
编辑了一个样本,其中包括71个Gev伽玛射线噪的活动星系核(14个BL Lac天体和57个平谱射电类星体),53个FRⅠ型射电星系和63个FRⅡ型射电星系.文章采用了非线性最小二乘法来拟合这个样本.当假设 M v =-23.0时,得到一个达到最佳拟合的哈勃常数,其拟合值为 H 0 =71.5±3.8kms -1Mpc -1.该值与通过哈勃望远镜关键计划所得到的哈勃常数值H 0=71.5±8 kms -1Mpc -1 符合得很好.其结果表明活动星系核的Gev伽玛辐射可以被用作宇宙标准烛光.
編輯瞭一箇樣本,其中包括71箇Gev伽瑪射線譟的活動星繫覈(14箇BL Lac天體和57箇平譜射電類星體),53箇FRⅠ型射電星繫和63箇FRⅡ型射電星繫.文章採用瞭非線性最小二乘法來擬閤這箇樣本.噹假設 M v =-23.0時,得到一箇達到最佳擬閤的哈勃常數,其擬閤值為 H 0 =71.5±3.8kms -1Mpc -1.該值與通過哈勃望遠鏡關鍵計劃所得到的哈勃常數值H 0=71.5±8 kms -1Mpc -1 符閤得很好.其結果錶明活動星繫覈的Gev伽瑪輻射可以被用作宇宙標準燭光.
편집료일개양본,기중포괄71개Gev가마사선조적활동성계핵(14개BL Lac천체화57개평보사전류성체),53개FRⅠ형사전성계화63개FRⅡ형사전성계.문장채용료비선성최소이승법래의합저개양본.당가설 M v =-23.0시,득도일개체도최가의합적합발상수,기의합치위 H 0 =71.5±3.8kms -1Mpc -1.해치여통과합발망원경관건계화소득도적합발상수치H 0=71.5±8 kms -1Mpc -1 부합득흔호.기결과표명활동성계핵적Gev가마복사가이피용작우주표준충광.
In this work,we compile a sample which contains 71 Gev Gamma-ray-loud Active Galactic Nuclei (AGNs)(14 BL Lacs and 57 FSRQs),53 FR Ⅰ radio galaxies and 63 FR Ⅱ radio galaxies.We make a nonlinear least-square fit to this sample,and find that the best fit value of the Hubble constant is H 0 =71.5±3.8km s -1 Mpc -1 with a reduced χ 22.46 by assuming M v =-23.0 and accepting q 0 =1.0,and the corresponding regression line has a correlation index R 0.78.The best fit value of H 0 =71.5±3.8 km s -1 Mpc -1 is in well agreement with H 0 =72±8 km s -1 obtained by the Hubble Space Telescope Key Project.Our results show that the Gev Gamma-ray emissions of AGNs can be used as cosmological standard candles indeed.