RESOLVING THE INNER JET STRUCTURE OF 1924-292 WITH THE EVENT HORIZON TELESCOPE | |
Lu, Ru-Sen1; Fish, Vincent L.1; Weintroub, Jonathan2; Doeleman, Sheperd S.1; Bower, Geoffrey C.3; Freund, Robert4; Friberg, Per; Ho, Paul T. P.5,6; Honma, Mareki7,8; Inoue, Makoto6 | |
刊名 | ASTROPHYSICAL JOURNAL LETTERS |
2012-09-20 | |
卷号 | 757期号:1页码:1 |
关键词 | galaxies: active galaxies: jets quasars: individual (1924-292) radio continuum: general techniques: high angular resolution techniques: interferometric |
英文摘要 | We present the first 1.3 mm (230 GHz) very long baseline interferometry model image of an active galactic nucleus (AGN) jet using closure phase techniques with a four-element array. The model image of the quasar 1924-292 was obtained with four telescopes at three observatories: the James Clerk Maxwell Telescope on Mauna Kea in Hawaii, the Arizona Radio Observatory's Submillimeter Telescope in Arizona, and two telescopes of the Combined Array for Research in Millimeter-wave Astronomy in California in 2009 April. With the greatly improved resolution compared with previous observations and robust closure phase measurement, the inner jet structure of 1924-292 was spatially resolved. The inner jet extends to the northwest along a position angle of -53 degrees. at a distance of 0.38 mas from the tentatively identified core, in agreement with the inner jet structure inferred from lower frequencies, and making a position angle difference of similar to 80 degrees with respect to the centimeter jet. The size of the compact core is 0.15 pc with a brightness temperature of 1.2 x 10(11) K. Compared with those measured at lower frequencies, the low brightness temperature may argue in favor of the decelerating jet model or particle-cascade models. The successful measurement of closure phase paves the way for imaging and time resolving Sgr A* and nearby AGNs with the Event Horizon Telescope. |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | ACTIVE GALACTIC NUCLEI ; COMPACT RADIO-SOURCES ; SAGITTARIUS A-ASTERISK ; GHZ VLBI SURVEY ; BRIGHTNESS TEMPERATURES ; SPECTRA ; CATALOG |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000308916900014 |
内容类型 | 期刊论文 |
源URL | [http://119.78.226.72/handle/331011/18074] |
专题 | 上海天文台_射电天文重点实验 |
作者单位 | 1.MIT, Haystack Observ, Westford, MA 01886 USA 2.Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA 3.Univ Calif Berkeley, Radio Astron Lab, Dept Astron, Berkeley, CA 94720 USA 4.Univ Arizona, Steward Observ, Arizona Radio Observ, Tucson, AZ 85721 USA 5.Joint Astron Ctr, James Clerk Maxwell Telescope, Hilo, HI 96720 USA 6.Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan 7.Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan 8.Grad Univ Adv Studies, Mitaka, Tokyo 1818588, Japan 9.Max Planck Inst Radioastron, D-53121 Bonn, Germany 10.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China |
推荐引用方式 GB/T 7714 | Lu, Ru-Sen,Fish, Vincent L.,Weintroub, Jonathan,et al. RESOLVING THE INNER JET STRUCTURE OF 1924-292 WITH THE EVENT HORIZON TELESCOPE[J]. ASTROPHYSICAL JOURNAL LETTERS,2012,757(1):1. |
APA | Lu, Ru-Sen.,Fish, Vincent L..,Weintroub, Jonathan.,Doeleman, Sheperd S..,Bower, Geoffrey C..,...&Zensus, J. Anton.(2012).RESOLVING THE INNER JET STRUCTURE OF 1924-292 WITH THE EVENT HORIZON TELESCOPE.ASTROPHYSICAL JOURNAL LETTERS,757(1),1. |
MLA | Lu, Ru-Sen,et al."RESOLVING THE INNER JET STRUCTURE OF 1924-292 WITH THE EVENT HORIZON TELESCOPE".ASTROPHYSICAL JOURNAL LETTERS 757.1(2012):1. |
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