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首页> 外文期刊>The Astrophysical journal >THE SPITZER c2d SURVEY OF NEARBY DENSE CORES. II. DISCOVERY OF A LOW-LUMINOSITY OBJECT IN THE 'EVOLVED STARLESS CORE' L1521f
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THE SPITZER c2d SURVEY OF NEARBY DENSE CORES. II. DISCOVERY OF A LOW-LUMINOSITY OBJECT IN THE 'EVOLVED STARLESS CORE' L1521f

机译:附近密密麻麻小店的SPITZER C2D调查。二。 “进化的繁星核心” L1521f中的低发光度对象的发现

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摘要

We present Spitzer Space Telescope observations of the "evolved starless core" L1521F that reveal the presence of a very low luminosity object (L < 0.07 solar luminosity). The object, L1521F-IRS, is directly detected at mid-infrared wavelengths ( > 5 μm), but only in scattered light at shorter infrared wavelengths, showing a bipolar nebula oriented east-west that is probably tracing an outflow cavity. The nebula strongly suggests that L1521F-IRS is embedded in the L1521F core. Thus, L1521F-IRS is similar to the recently discovered L1014-IRS and the previously known IRAM 04191 in its substellar luminosity and dense core environment. However, these objects differ significantly in their core density, core chemistry, and outflow properties, and some may be destined to be brown dwarfs rather than stars.
机译:我们展示了“未演化的恒星核心” L1521F的Spitzer太空望远镜观测结果,该观测结果表明存在一个非常低的发光度物体(L <0.07太阳发光度)。 L1521F-IRS是在中红外波长(> 5μm)上直接检测到的,但仅在较短的红外波长的散射光下才能检测到,显示了一个双极星云取向的东西向,可能正在追踪流出腔。星云强烈暗示L1521F-IRS嵌入在L1521F核心中。因此,L1521F-IRS在星下发光度和密集核心环境方面类似于最近发现的L1014-IRS和先前已知的IRAM 04191。但是,这些天体的核心密度,核心化学性质和流出特性存在显着差异,并且可能注定是褐矮星而不是恒星。

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