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首页> 外文期刊>The Astrophysical journal >LIFETIMES OF ULTRACOMPACT H II REGIONS: HIGH-RESOLUTION METHYL CYANIDE OBSERVATIONS
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LIFETIMES OF ULTRACOMPACT H II REGIONS: HIGH-RESOLUTION METHYL CYANIDE OBSERVATIONS

机译:超紧凑H II区的寿命:高分辨率甲基氰化物的观测

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摘要

We observed the dense molecular cores associated with two ultracompact H II regions, G5.89 + 0.4 and G34.3 + 0.2, in the J = 6-5 transitions of CH_3CN to probe the temperature and density of the gas. Simultaneously, each region was observed in the J = 1-0 transition of a CO isotope to probe the molecular column density. The molecular cores are found to have densities ~10~6 cm~(-3) and kinetic temperatures of 90 and 250 K, respectively. We also find possible evidence for infall of molecular gas toward the H II regions. The lifetime of the H II region ultracompact phase is critically dependent on the properties of the surrounding molecular gas. Based on the number of ultracompact H II regions versus the total number of O stars, it has been suggested that the lifetime of the ultracompact phase is inconsistent with spherical expansion confined only by the ambient medium. We show that for the molecular cloud parameters given above and including the effect of the shell of neutral material formed by the expansion, pressure confinement by the ambient medium may significantly increase the lifetime of the ultracompact phase of the H II regions.
机译:我们在CH_3CN的J = 6-5跃迁中观察到与两个超紧凑型H II区G5.89 + 0.4和G34.3 + 0.2相关的致密分子核,以探测气体的温度和密度。同时,在CO同位素的J = 1-0跃迁中观察到每个区域,以探测分子柱密度。发现分子核的密度分别为〜10〜6 cm〜(-3),动力学温度分别为90 K和250K。我们还发现分子气体进入H II区的可能证据。 H II区超致密相的寿命主要取决于周围分子气体的特性。基于超紧凑H II区域的数量与O星总数的比较,已经表明,超紧凑相的寿命与仅由环境介质限制的球形膨胀不一致。我们表明,对于上面给出的分子云参数,包括由膨胀形成的中性材料壳的影响,环境介质的压力限制可能会显着增加H II区超致密相的寿命。

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