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相关论文: 3.3 {\mu}m PAH observations of the central kilopar…

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Based on recent results obtained by the Pierre Auger Observatory (PAO), it has been hypothesized that Centaurus A (Cen A) is a source of ultra-high-energy cosmic rays (UHECRs) and associated neutrinos. We point out that the diffuse neutrino…

天体物理学 · 物理学 2010-04-21 Hylke B. J. Koers , Peter Tinyakov

We investigate the mid-infrared radiation of galaxies that are powered by a starburst or by an AGN. For this end, we compare the spectra obtained at different spatial scales in a sample of infrared bright galaxies. ISO observations which…

天体物理学 · 物理学 2008-12-18 R. Siebenmorgen , E. Kr"ugel , H. W. W. Spoon

Infrared emission features at 3.3, 6.2, 7.7, 8.6, and 11.2 $\mu$m, attributed to polycyclic aromatic hydrocarbons, show variations in relative intensity, shape, and peak position. These variations depend on the physical conditions of the…

星系天体物理 · 物理学 2021-11-24 C. Knight , E. Peeters , M. Wolfire , D. J. Stock

The interstellar medium of Centaurus A (NGC 5128) has been studied extensively in recent years, using mostly molecular lines tracing low to medium density gas (500 to several $10^3$ cm$^{-3}$). The amount and distribution of the dense…

天体物理学 · 物理学 2007-05-23 W. Wild , A. Eckart

Due to its proximity and its importance for the understanding of active galaxies and their active nuclei (AGN), Centaurus A has been observed frequently within the last 150 years in all accessible wavelength bands. Thus a wealth of data…

天体物理学 · 物理学 2009-11-06 Helmut Steinle

We present a detailed study of the complex ionization structure in a small (~250 pc) extended narrow line region (ENLR) cloud near Centaurus A using the Multi Unit Spectroscopic Explorer. This cloud is located in the so-called outer…

星系天体物理 · 物理学 2016-05-04 F. Santoro , J. B. R. Oonk , R. Morganti , T. A. Oosterloo , C. Tadhunter

We present a sample of low-resolution 5-38um Spitzer IRS spectra of the inner few square kiloparsecs of 59 nearby galaxies spanning a large range of star formation properties. A robust method for decomposing mid-infrared galaxy spectra is…

Centaurus A is the closest active galactic nucleus. High resolution imaging using Very Long Baseline Interferometry (VLBI) enables us to study the spectral and kinematic behavior of the radio jet-counterjet system on sub-parsec scales,…

EGRET has detected 67 sources associated with active galactic nuclei. With the exception of radio galaxy Cen A, all are classified as belonging to the blazar class of active galactic nuclei. The cumulative exposure from multiple EGRET…

天体物理学 · 物理学 2010-12-03 P. Sreekumar , D. L. Bertsch , R. C. Hartman , P. L. Nolan , D. J. Thompson

The non-thermal emission from the kiloparsec-scale jet of Centaurus A exhibits two notable features, bright diffuse emission and many compact knots, which have been intensively studied in X-ray and radio observations. H.E.S.S. recently…

高能天体物理现象 · 物理学 2020-10-07 Takahiro Sudoh , Dmitry Khangulyan , Yoshiyuki Inoue

We used the near infrared spectrometer ISAAC at the ESO 'Very Large Telescope' to map the velocity field of Centaurus A (NGC 5128) at several position angles and locations in the central 20" of the galaxy. The high spatial resolution…

We report on infrared K- (2-2.5 micron) and L-band (2.8-4.1 micron) slit spectroscopy of 23 Seyfert 1 galaxies in the CfA and 12 micron samples. A polycyclic aromatic hydrocarbon (PAH) emission feature at 3.3 micron in the L band is…

天体物理学 · 物理学 2009-11-10 Masatoshi Imanishi , Keiichi Wada

We have performed IRS low resolution 5-12 micron spectroscopy on a sample of galaxies selected to be at 3 distinct post-starburst evolutionary stages based on their optical spectral indices. The resulting IRS spectra show distinctive PAH…

宇宙学与河外天体物理 · 物理学 2011-02-11 I. G. Roseboom , S. Oliver , D. Farrah

We present spatial distribution of polycyclic aromatic hydrocarbons and ionized gas within the Galactic giant HII region NGC3603. Using the IRS instrument on board the Spitzer Space Telescope, we study in particular the PAH emission…

天体物理学 · 物理学 2009-06-23 V. Lebouteiller , B. Brandl , J. Bernard-Salas , D. Devost , J. R. Houck

The main purpose of this research was to investigate how energetic processes associated with Active Galactic Nuclei are related to those due to nuclear or circumnuclear star formation activity. Photometric and spectroscopic data were used…

宇宙学与河外天体物理 · 物理学 2013-08-07 Mario-A Higuera-G , Andres F. Ramos P

We present J, H and K-band images and 0.9-2.5 micron spectra of the nuclear regions of Centaurus A obtained with IRIS on the AAT. While K band has a point source coincident with the nucleus, at H and J we identify diffuse structure…

天体物理学 · 物理学 2009-10-31 J. J. Bryant , R. W. Hunstead

We present Spitzer/Infrared Spectrograph (IRS) 5-21 micron spectroscopic maps towards 12 regions in the Andromeda galaxy (M31). These regions include the nucleus, bulge, an active region in the star-forming ring, and 9 other regions chosen…

We discuss the possibility that a dominant fraction of the cosmic rays above the ankle is due to a single nearby source, considering in particular the radio galaxy Centaurus A. We focus on the properties of the source spectrum and…

高能天体物理现象 · 物理学 2024-11-28 Silvia Mollerach , Esteban Roulet

The ultra--high energy cosmic rays recently detected by several air shower experiments could have an extragalactic origin. In this case, the nearest active galaxy Centaurus A might be the source of the most energetic particles ever detected…

广义相对论与量子宇宙学 · 物理学 2011-05-23 G. E. Romero , J. A. Combi , S. E. Perez Bergliaffa , L. A. Anchordoqui

We present new HST/STIS observations of Centaurus A. [SIII] 9533A was used to study the kinematics in the nuclear region with a 0.1" spatial resolution. The STIS data and the VLT/ISAAC spectra by Marconi et al. (2001) provide independent…

天体物理学 · 物理学 2009-11-11 A. Marconi , G. Pastorini , F. Pacini , D. J. Axon , A. Capetti , D. Macchetto , A. M. Koekemoer , E. J. Schreier