Academic Journal
Kinematics and Chemistry of the Hot Molecular Core in G34.26+0.15 at High Resolution
العنوان: | Kinematics and Chemistry of the Hot Molecular Core in G34.26+0.15 at High Resolution |
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المؤلفون: | B. Mookerjea, E. Casper, L. G. Mundy, L. W. Looney |
المساهمون: | The Pennsylvania State University CiteSeerX Archives |
المصدر: | http://arxiv.org/pdf/astro-ph/0701827v1.pdf. |
سنة النشر: | 2007 |
المجموعة: | CiteSeerX |
الوصف: | We present high angular resolution ( ∼ 1 ′ ′ ) multi-tracer spectral line observations toward the hot core associated with G34.26+0.15 between 87–109 GHz. We have mapped emission from (i) complex nitrogen- and oxygen-rich molecules like CH3OH, HC3N, CH3CH2CN, NH2CHO, CH3OCH3, HCOOCH3; (ii) sulfurbearing molecules like OCS, SO and SO2; and (iii) the recombination line H53β. The high angular resolution enables us to directly probe the hot molecular core associated with G34.26+0.15 at spatial scales of 0.018 pc. At this resolution we find no evidence for the hot core being internally heated. The continuum peak detected at λ = 2.8 mm is consistent with the free-free emission from component C of the ultracompact H ii region. Velocity structure and morphology outlined by the different tracers suggest that the hot core is primarily energized by component C. Emission from the N- and O-bearing molecules peak at different positions within the innermost regions of the core; none are coincident with the continuum peak. Lack of high resolution complementary datasets makes |
نوع الوثيقة: | text |
وصف الملف: | application/pdf |
اللغة: | English |
Relation: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.316.5687; http://arxiv.org/pdf/astro-ph/0701827v1.pdf |
الاتاحة: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.316.5687 http://arxiv.org/pdf/astro-ph/0701827v1.pdf |
Rights: | Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
رقم الانضمام: | edsbas.340B9487 |
قاعدة البيانات: | BASE |
الوصف غير متاح. |