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光学微弱的微央斯基射电源。

Optically Faint Microjansky Radio Sources.

作者信息

Richards EA, Fomalont EB, Kellermann KI, Windhorst RA, Partridge RB, Cowie LL, Barger AJ

出版信息

Astrophys J. 1999 Dec 1;526(2):L73-L76. doi: 10.1086/312373.

Abstract

We report on the identifications of radio sources from our survey of the Hubble Deep Field (HDF) and the Small Selected Area 13 fields, both of which comprise the deepest radio surveys to date at 1.4 and 8.5 GHz, respectively. About 80% of the microjansky radio sources are associated with moderate-redshift starburst galaxies or active galactic nuclei within the I-magnitude range of 17-24 with a median of I=22 mag. Thirty-one (20%) of the radio sources are (1) fainter than I>25 mag, with two objects in the HDF IAB>28.5, (2) often identified with very red objects I-K>4, and (3) not significantly different in radio properties than the brighter objects. We suggest that most of these objects are associated with heavily obscured starburst galaxies with redshifts between 1 and 3. However, other mechanisms are discussed and cannot be ruled out with the present observations.

摘要

我们报告了在对哈勃深场(HDF)和小选定区域13场进行的调查中对射电源的识别情况,这两个区域分别是迄今为止在1.4 GHz和8.5 GHz频率下最深的射电调查。约80%的微央斯基射电源与I星等范围在17至24(中位数为I = 22星等)之间的中等红移星暴星系或活动星系核相关。31个(20%)射电源(1)比I > 25星等更暗,哈勃深场中有两个物体的IAB > 28.5,(2)常与极红物体(I - K > 4)相关,(3)在射电特性上与较亮物体没有显著差异。我们认为这些物体中的大多数与红移在1至3之间的高度遮蔽星暴星系相关。然而,也讨论了其他机制,并且目前的观测不能排除这些机制。

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