Tracing PAH Emission in λ-Orionis Using COBE/DIRBE Data
نویسندگان
چکیده
We use archival COBE/DIRBE data to construct a map of polycyclic aromatic hydrocarbon (PAH) emission in the $\lambda$-Orionis region. The presence 3.3 $\mu$m PAH feature within DIRBE 3.5 band and corresponding lack significant spectral features adjacent bands (1.25, 2.2, 4.9 $\mu$m) enable estimation contribution data. Having shortest wavelength known features, probes smallest PAHs, which are also leading candidates for carriers anomalous microwave (AME). this investigate association between AME from molecules. find that spatial correlation is higher far-infrared dust (as represented by 240 map) than it our AME. This finding, agreement with previous studies using at longer wavelengths, tension hypothesis due spinning PAHs. However, expected mid-infrared could potentially be degraded different sensitivities each mechanism local environmental conditions even if PAHs both.
منابع مشابه
The λ-Orionis Ring in CO
The results of a new CO(J=1→0) survey of the ring of molecular clouds around the H ii region Sh-2-264 and the λ-Orionis OB-association are presented. The distribution of molecular gas closely approximates that of the dust seen in IRAS emission. The total molecular mass is 1.4×104 M . The mass spectrum of the emission clumps is a power-law with index -1.8, similar to that observed in other star-...
متن کاملpattern recognition in maintenance data using methodologies data minitng (cade study isfahan regional power electric company)
فعالیت های نگهداری و تعمیرات اطلاعاتی را تولید می کند که می تواند در تعیین زمان های بیکاری و ارایه یک برنامه زمان بندی شده یا تعیین هشدارهای خرابی به پرسنل نگهداری و تعمیرات کمک کند. وقتی که مقدار داده های تولید شده زیاد باشند، فهم بین متغیرها بسیار مشکل می شوند. این پایان نامه به کاربردی از داده کاوی برای کاوش پایگاه های داده چندبعدی در حوزه نگهداری و تعمیرات، برای پیدا کردن خرابی هایی که موجب...
15 صفحه اولUnusual PAH Emission in Elliptical Galaxies
In a sample of thirty normal elliptical galaxies observed with the Spitzer IRS, one galaxy, NGC4697, shows strong PAH emission, but with an apparently weak 7.7 μm feature. We find that the PAH emission is confined to the central regions of the galaxy and that once a quiescent elliptical galaxy spectrum is subtracted, the PAH feature ratios are normal. We show that the PAH spectrum resembles the...
متن کاملPAH emission from Herbig AeBe stars
We present spectra of a sample of Herbig Ae and Be (HAeBe) stars obtained with the Infrared Spectrograph on the Spitzer Space Telescope. All but one of the Herbig stars show emission from polycyclic aromatic hydrocarbons (PAHs) and seven of the spectra show PAH emission, but no silicate emission at 10 μm. The central wavelengths of the 6.2, 7.7–8.2, and 11.3 μm emission features decrease with s...
متن کاملPah Emission from Ultraluminous Infrared Galaxies
We explore the relationships between the Polycyclic Aromatic Hydrocarbon (PAH) feature strengths, mid-infrared continuum luminosities, far-infrared spectral slopes, optical spectroscopic classifications, and silicate optical depths within a sample of 107 ULIRGs observed with the Infrared Spectrograph on the Spitzer Space Telescope. The detected 6.2 μm PAH equivalent widths (EQWs) in the sample ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2022
ISSN: ['2041-8213', '2041-8205']
DOI: https://doi.org/10.3847/1538-4357/ac9b24