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相关论文: Dusty Superwind from a Galaxy with a Compact Obscu…

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High resolution, Hubble Space Telescope (HST) near-infrared and Keck mid-infrared images of the heavily extinguished, infrared luminous galaxy NGC 4418 are presented. These data make it possible to observe the imbedded near-infrared…

The galaxy NGC 4418 contains one of the most compact obscured nuclei within a luminous infrared galaxy (LIRG) in the nearby Universe. This nucleus contains a rich molecular gas environment and an unusually high ratio of infrared to radio…

星系天体物理 · 物理学 2014-06-04 E. Varenius , J. E. Conway , I. Martí-Vidal , S. Aalto , R. Beswick , F. Costagliola , H. -R. Klöckner

We have observed the nucleus of the nearby luminous infrared galaxy NGC 4418 with subarcsec resolution at 860 and 450 micron for the first time to characterize its hidden power source. A ~20 pc (0.1") hot dusty core was found inside a 100…

宇宙学与河外天体物理 · 物理学 2015-06-12 Kazushi Sakamoto , Susanne Aalto , Francesco Costagliola , Sergio Martin , Youichi Ohyama , Martina C. Wiedner , David J. Wilner

The aim of this study is to constrain the dynamics, structure and feeding of the compact nucleous of NGC4418, and to reveal the nature of the main hidden power source: starburst or AGN. We obtained high spatial resolution observations of…

星系天体物理 · 物理学 2015-06-16 F. Costagliola , S. Aalto , K. Sakamoto , S. Martín , R. Beswick , S. Muller , H. -R. Klöckner

We performed deep spectropolarimetric observations of a prototypical starburst galaxy M82 with the Subaru Telescope in order to study the kinematics of the dust outflow. We obtained optical polarized emission-line spectra up to $\sim$4~kpc…

星系天体物理 · 物理学 2019-08-21 Michitoshi Yoshida , Koji S. Kawabata , Youichi Ohyama , Ryosuke Itoh , Takashi Hattori

Spectropolarimetry results for the starburst galaxy M82 are presented. The optical emission lines of the filaments in the energetic outflow ("superwind") from the nuclear starburst region of M82 are substantially polarized. The H-alpha…

宇宙学与河外天体物理 · 物理学 2015-05-20 Michitoshi Yoshida , Koji S. Kawabata , Youichi Ohyama

We have thoroughly characterized the ultraviolet to near-infrared (0.15 - 2.2 micron) spectral energy distribution (SED) of the central parsec of the M33 nucleus through new infrared photometry and optical/near-infrared spectroscopy,…

天体物理学 · 物理学 2016-08-30 K. D. Gordon , M. M. Hanson , G. C. Clayton , G. H. Rieke , K. A. Misselt

Multi-wavelength images from the Hubble Space Telescope covering the wavelength range 0.27-1.6 $\mu$m show that the central area of the nearby dwarf galaxy NGC4449 contains several tens of compact sources that are emitting in the hydrogen…

We report the detection of absorption features in the 6-8 micron region superimposed on a featureless mid-infrared continuum in NGC 4418. For several of these features this is the first detection in an external galaxy. We compare the…

天体物理学 · 物理学 2009-10-31 H. W. W. Spoon , J. V. Keane , A. G. G. M. Tielens , D. Lutz , A. F. M. Moorwood

We present near-infrared and millimeter investigations of the nucleus of the infrared luminous galaxy NGC 4418, which previous observations suggest possesses a powerful buried AGN. We found the following main results: (1) The infrared…

天体物理学 · 物理学 2009-11-10 Masatoshi Imanishi , Kouichiro Nakanishi , Nario Kuno , Kotaro Kohno

We present a detailed analysis of deep far-infrared observations of the nearby edge-on star-forming galaxy NGC 4631 obtained with the Herschel Space Observatory. Our PACS images at 70 and 160 um show a rich complex of filaments and…

Compact obscured nuclei (CONs) are an extremely obscured (N$_{H2}$ >10$^{25}$ cm$^{-2}$) class of galaxy nuclei thought to exist in 20-40 per cent of nearby (ultra-)luminous infrared galaxies. While they have been proposed to represent a…

We present new observations of the famous starburst galaxy NGC 5253 which owes its celebrity to possibly being the youngest and closest starburst galaxy known. Our observations in the infrared and millimeter contribute to shed light on the…

天体物理学 · 物理学 2016-08-30 Leonardo Vanzi , Marc Sauvage

(Abridged) We combine NUV, optical and IR imaging of the nearby starburst galaxy M82 to explore the properties of the dust both in the interstellar medium of the galaxy and the dust entrained in the superwind. The three NUV filters of…

星系天体物理 · 物理学 2015-06-18 S. Hutton , I. Ferreras , K. Wu , N. P. M. Kuin , A. Breeveld , V. Yershov , M. Cropper , M. J. Page

The composite galaxy NGC 4102 hosts a LINER nucleus and a starburst. We mapped NGC 4102 in the 12.8 micron line of [NeII], using the echelon spectrometer TEXES on the NASA IRTF, to obtain a data cube with 1.5" spatial and 25 km/s spectral,…

星系天体物理 · 物理学 2015-05-19 Sara C. Beck , John H. Lacy , Jean L. Turner

We present results from a 30 ksec Chandra observation of the important starburst galaxy NGC 2782, covering the 0.3-10keV energy band. We find evidence of a superwind of small extent, that is likely in an early stage of development. We find…

星系天体物理 · 物理学 2017-03-22 Jimena Bravo-Guerrero , Ian R. Stevens

The 9.7-micron silicate absorption profile in the interstellar medium provides important information on the physical and chemical composition of interstellar dust grains. Measurements in the Milky Way have shown that the profile in the…

星系天体物理 · 物理学 2015-06-24 P. F. Roche , A. Alonso-Herrero , O. Gonzalez-Martin

The central 2x1 kpc of the starburst galaxy NGC 253 has been imaged using the Submillimeter Array at a 60 pc resolution in the J=2-1 transitions of 12CO, 13CO, and C18O as well as in the 1.3 mm continuum. Molecular gas and dust are mainly…

NGC 2146, a nearby luminous infrared galaxy (LIRG), presents evidence for outflows along the disk minor axis in all gas phases (ionized, neutral atomic and molecular). We present an analysis of the multi-phase starburst driven superwind in…

Compact obscured nuclei (CONs) are relatively common in the centers of local (U)LIRGs, yet their nature remains unknown. Both AGN activity and extreme nuclear starbursts have been suggested as plausible nuclear power sources. The prevalence…

星系天体物理 · 物理学 2023-09-06 C. F. Wethers , S. Aalto , G. C. Privon , F. Stanley , J. Gallagher , M. Gorski , S. König , K. Onishi , C. Yang
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