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相关论文: Comparing Infrared Star-Formation Rate Indicators …

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We present an analysis of the mid-infrared spectra, obtained from the Spitzer Space Telescope, of the dark globule, DC 314.8--5.1, which is at the onset of low-mass star formation. The target has a serendipitous association with a B-type…

星系天体物理 · 物理学 2022-08-03 E. Kosmaczewski , Ł. Stawarz , W. R. M. Rocha , S. S. Shenoy , A. Karska

Hydrocarbon dust is one of the dominant components of interstellar dust, which mainly consists of polycyclic aromatic hydrocarbons and aliphatic hydrocarbons. While hydrocarbon dust is thought to be processed in interstellar radiation…

This study presents optical and near-infrared photometric observations, alongside mid-infrared spectroscopic data from the ISO SWS instrument, to examine potential correlations between Aromatic Infrared Band (AIB) features and the optical…

星系天体物理 · 物理学 2025-08-08 Rahul Kumar Anand , Atul Kumar Singh , Saurabh Sharma , Brijesh Kumar , Shantanu Rastogi

In this paper we analyze the evolution of actively star forming galaxies in the mid-infrared (MIR). This spectral region, characterized by continuum emission by hot dust and by the presence of strong emission features generally ascribed to…

天体物理学 · 物理学 2016-08-30 O. Vega , L. Silva , P. Panuzzo , A. Bressan , G. L. Granato , M. Chavez

Polycyclic Aromatic Hydrocarbons (PAHs) are carbon-based molecules resulting from the union of aromatic rings and related species, which are likely responsible for strong infrared emission features (3.3, 6.2, 7.7, 8.6, 11.3 and 12.7…

星系天体物理 · 物理学 2021-11-05 I. García-Bernete , D. Rigopoulou , A. Alonso-Herrero , M. Pereira-Santaella , P. F. Roche , B. Kerkeni

We present Spitzer rest-frame mid-infrared spectroscopy of twelve z~2 mm-bright type 1 QSOs, selected from unlensed and lensed QSO samples and covering a range of AGN optical luminosities L_5100=10^45 to 10^47 erg/s. On top of the AGN…

Polycyclic Aromatic Hydrocarbons (PAHs) are considered as a major constituent of interstellar dust. They have been proposed as the carriers of the Aromatic Infrared Bands (AIBs) observed in emission in the mid-IR. They likely have a…

星系天体物理 · 物理学 2009-04-22 C. Joblin , O. Berne , A. Simon , G. Mulas

We present a study of a large, statistically complete sample of star-forming dwarf galaxies using mid-infrared observations from the {\it Spitzer Space Telescope}. The relationships between metallicity, star formation rate (SFR) and…

星系天体物理 · 物理学 2010-07-01 Sukbum A. Hong , Jessica L. Rosenberg , Matthew L. N. Ashby , John J. Salzer

Evolutionary properties of infrared (IR) luminous galaxies are important keys to understand dust-obscured star formation history and galaxy evolution. Based on the near- to mid-IR imaging with 9 continuous filters of AKARI space telescope,…

We present a sample of resolved galactic HII regions and photodissociation regions (PDRs) observed with the Spitzer infrared spectrograph (IRS) in spectral mapping mode between the wavelengths of 5--15 $\mu$m. For each object we have…

Using the Mid-Infrared Spectrometer on board the Infrared Telescope in Space and the low-resolution grating spectrometer (PHT-S) on board the Infrared Space Observatory, we obtained 820 mid-infrared (5 to 12 $\mu$m) spectra of the diffuse…

天体物理学 · 物理学 2009-10-31 Kin-Wing Chan , T. L. Roellig , T. Onaka , M. Mizutani , K. Okumura , I. Yamamura , T. Tanabe , H. Shibai , T. Nakagawa , H. Okuda

We use JWST/NIRCam and MIRI imaging acquired by the Feedback in Emerging extrAgalactic Star clusTers (FEAST) program along with archival HST imaging to map ionized gas (Pa$\alpha$, Br$\alpha$, and H$\alpha$) and Polycyclic Aromatic…

The mid-infrared (IR) range contains many spectral features associated with large molecules and dust grains such as polycyclic aromatic hydrocarbons (PAHs) and silicates. These are usually very strong compared to fine-structure gas lines,…

I summarize the results of two recent studies, based on ISO and Spitzer mid-IR spectra of galaxies and Galactic regions, aimed at understanding the origins of the variations of the aromatic features among and inside galaxies. I show that…

天体物理学 · 物理学 2007-05-23 F. Galliano

The mid-infrared (MIR) spectra of dense photodissociation regions (PDRs) are typically dominated by emission from polycyclic aromatic hydrocarbons (PAHs) and the lowest pure rotational states of molecular hydrogen (H2); two species which…

星系天体物理 · 物理学 2011-02-09 Brian T. Fleming , Kevin France , Roxana E. Lupu , Stephan R. McCandliss

We use HST NICMOS continuum and Pa-alpha observations to study the near-infrared and star-formation properties of a representative sample of 30 local (d ~ 35-75Mpc) luminous infrared galaxies (LIRGs, infrared 8-1000um luminosities of…

天体物理学 · 物理学 2008-11-26 A. Alonso-Herrero , G. H. Rieke , M. J. Rieke , L. Colina , P. G. Perez-Gonzalez , S. D. Ryder

We investigate the global cold dust properties of 85 nearby (z < 0.5) QSOs, chosen from the Palomar-Green sample of optically luminous quasars. We determine their infrared spectral energy distributions and estimate their rest-frame…

星系天体物理 · 物理学 2015-08-19 Andreea O. Petric , Luis C. Ho , Nicolas J. M. Flagey , Nicholas Z. Scoville

We present mid-infrared to optical properties of 22 representative irregular galaxies: 18 Im, 3 BCDs, and one Sm. The mid-IR is based on images from the Spitzer Space Telescope archives. The 3.6 and 4.5 micron bands and the UBVJHK images…

天体物理学 · 物理学 2008-11-26 Deidre A. Hunter , Bruce G. Elmegreen , Emily Martin

The relationships between atomic and molecular hydrogen and dust of various sizes in extragalactic star-forming regions are considered, based on observational data from the Spitzer and Herschel infrared space telescopes, the Very Large…

星系天体物理 · 物理学 2017-12-07 K. I. Smirnova , M. S. Murga , D. S. Wiebe , A. M. Sobolev

Mixtures of polycylic aromatic hydrocarbons (PAHs) have been produced by means of laser pyrolysis. The main fraction of the extracted PAHs were primarily medium-sized, up to a maximum size of 38 carbon atoms per molecule. The use of…

天体物理仪器与方法 · 物理学 2011-01-24 M. Steglich , C. Jäger , G. Rouillé , F. Huisken , H. Mutschke , Th. Henning