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相关论文: Deep JHKs and Spitzer Imaging of Four Isolated Mol…

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The extinction curve of interstellar dust in the dense molecular cloud cores is crucial for understanding dust properties, particularly size distribution and composition. We investigate the infrared extinction law in four nearby isolated…

星系天体物理 · 物理学 2024-11-04 Jun Li , Bingqiu Chen , Biwei Jiang , He Zhao , Botao Jiang , Xi Chen

The relation between ices in the envelopes and disks surrounding YSOs and those in the quiescent interstellar medium is investigated. For a sample of 31 stars behind isolated dense cores, ground-based and Spitzer spectra and photometry in…

We compute the mid-infrared extinction law from 3.6-24 microns in three molecular clouds: Ophiuchus, Perseus, and Serpens, by combining data from the "Cores to Disks" Spitzer Legacy Science program with deep JHKs imaging. Using a new…

天体物理学 · 物理学 2008-12-18 Nicholas L. Chapman , Lee G. Mundy , Shih-Ping Lai , Neal J. Evans

Context. The properties of dust grains, in particular their size distribution, are expected to differ from the interstellar medium to the high-density regions within molecular clouds. Aims. We measure the mid-infrared extinction law…

星系天体物理 · 物理学 2015-06-12 J. Ascenso , C. J. Lada , J. Alves , C. G. Román-Zúñiga , M. Lombardi

We present an independent estimate of the interstellar extinction law for the Spitzer IRAC bands as well as a first attempt at extending the law to the 24micron MIPS band. The source data for these measurements are observations of five…

天体物理学 · 物理学 2011-02-11 K. M. Flaherty , J. L. Pipher , S. T. Megeath , E. M. Winston , R. A. Gutermuth , J. Muzerolle , G. G. Fazio

(Abridged) We use 8 micron Spitzer GLIMPSE images to make extinction maps of 10 IRDCs, selected to be relatively nearby and massive. The extinction mapping technique requires modeling the IR background intensity behind the cloud, which is…

天体物理学 · 物理学 2011-02-11 Michael J. Butler , Jonathan C. Tan

Deep JHKs photometry was obtained towards eight dense molecular cores and J-H vs. H-Ks color-color plots are presented. Our photometry, sensitive to the detection of a 1 solar mass, 1 X 10^6 year old star through approx. 35 - 50 magnitudes…

天体物理学 · 物理学 2009-11-07 David C. Murphy , Philip C. Myers

Investigating the extinction properties in dense molecular clouds is of significant importance for understanding the behavior of interstellar dust and its impact on observations. In this study, we comprehensively examined the extinction law…

星系天体物理 · 物理学 2023-08-02 Jun Li , Xi Chen

This paper presents results from modelling 450 micron and 850 micron continuum and HCO+ line observations of three distinct cores of an infrared dark cloud (IRDC) directed toward the W51 GMC. In the sub-mm continuum these cores appear as…

天体物理学 · 物理学 2009-11-11 C. W. Ormel , R. F. Shipman , V. Ossenkopf , F. P. Helmich

A precise measure of the mid-infrared interstellar extinction law is crucial to the investigation of the properties of interstellar dust, especially of the grains in the large size end. Based on the stellar parameters derived from the…

星系天体物理 · 物理学 2016-11-10 Mengyao Xue , Biwei Jiang , Jian Gao , Jiaming Liu , Shu Wang , Aigen Li

We present Spitzer observations of a sample of 12 starless cores selected to have prominent 24 micron shadows. The Spitzer images show 8 and 24 micron shadows and in some cases 70 micron shadows; these spatially resolved absorption features…

A powerful way to observe directly the solid state inventory of dense molecular clouds is by infrared spectroscopy of background stars. We present Spitzer/IRS 5-20 micron spectra of ices toward stars behind the Serpens and Taurus molecular…

Context. The properties of dust grains, in particular their size distribution, are expected to differ from the interstellar medium to the high-density regions within molecular clouds. Since the extinction at near-infrared wavelengths is…

星系天体物理 · 物理学 2015-06-04 Joana Ascenso , Marco Lombardi , Charles J. Lada , João Alves

Tracing dust in small dense molecular cores is a powerful tool to study the conditions required for ices to form during the pre-stellar phase. To study these environments, five molecular cores were observed: three with ongoing low-mass star…

星系天体物理 · 物理学 2021-09-08 Laurie E. U. Chu , Klaus W. Hodapp

A precise extinction law is a critical input when interpreting observations of highly reddened sources such as young star clusters and the Galactic Center (GC). We use Hubble Space Telescope observations of a region of moderate extinction…

星系天体物理 · 物理学 2018-03-14 M. W. Hosek , J. R. Lu , J. Anderson , T. Do , E. F. Schlafly , A. M. Ghez , W. I. Clarkson , M. R. Morris , S. M. Albers

We have carried out near-infrared polarimetry toward the boundary of the Central Molecular Zone, in the field of (-1.4 deg $\lesssim l \lesssim$ -0.3 deg and 1.0 deg $\lesssim l \lesssim$ 2.9 deg, $|b|\lesssim$ 0.1 deg), using the…

星系天体物理 · 物理学 2015-06-19 Tatsuhito Yoshikawa , Shogo Nishiyama , Motohide Tamura , Jungmi Kwon , Tetsuya Nagata

Forty molecular cloud cores in the southern hemisphere from the initial Spitzer Space Telescope Cores-to-Disks (c2d) Legacy program source list have been surveyed in 13CO(2-1), 12CO(4-3), and 12CO(7-6) with the Antarctic Submillimeter…

天体物理学 · 物理学 2009-11-13 A. Loehr , T. L. Bourke , A. P. Lane , P. C. Myers , S. C. Parshley , A. A. Stark , N. F. H. Tothill

We use deep $8\:\mu m$ Spitzer-IRAC imaging of a massive Infrared Dark Cloud (IRDC) G028.37+00.07 to construct a Mid-Infrared (MIR) extinction map that probes mass surface densities up to $\Sigma\:\sim 1\:\rm{g~cm^{-2}}$…

太阳与恒星天体物理 · 物理学 2015-06-18 Michael J. Butler , Jonathan C. Tan , Jouni Kainulainen

Investigating the extinction law in regions of high dust extinction, such as the Pillars of Creation within the M16 region, is crucial for understanding the densest parts of the interstellar medium (ISM). In this study, we utilize…

星系天体物理 · 物理学 2024-06-06 Jun Li , Bingqiu Chen , Biwei Jiang , Jian Gao , Xi Chen

Context. The largest grains (0.5-1 micron) in the interstellar size distribution are efficient in scattering near- and mid-infrared radiation. These wavelengths are therefore particularly well suited to probe the still uncertain high-end of…

星系天体物理 · 物理学 2015-06-17 M. Andersen , J. Steinacker , W-F. Thi , L. Pagani , A. Bacmann , R. Paladini
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