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相关论文: NGC 4102: High Resolution Infrared Observations of…

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We present Gemini/GNIRS spectroscopy of the Seyfert 2 galaxy NGC 4388, with simultaneous coverage from 0.85 - 2.5 $\mu$m. Several spatially-extended emission lines are detected for the first time, both in the obscured and unobscured portion…

The infrared spectra of starburst galaxies are dominated by the low-excitation lines of [NeII] and [SIII], and the stellar populations deduced from these spectra appear to lack stars larger than about 35 Msun. The only exceptions to this…

天体物理学 · 物理学 2009-06-23 Sara C. Beck , Jean L. Turner , Jenna Kloosterman

We present near-infrared VLT ISAAC imaging and spectroscopy of the peculiar Virgo galaxy NGC 4438, whose nucleus has been classified as a LINER. The data are supplemented by mid-infrared imaging, and compared to previous WFPC2 HST broadband…

星系天体物理 · 物理学 2015-05-14 Sebastian Perez , Simon Casassus , Juan R. Cortes , J. D. P. Kenney

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…

NGC 4314 is an early-type barred galaxy containing a nuclear ring of recent star formation. We present CO(1-0) interferometer data of the bar and circumnuclear region with 2.3 x 2.2 arcsec spatial resolution and 13 km/s velocity resolution…

天体物理学 · 物理学 2009-10-28 G. Fritz Benedict , Beverly J. Smith , Jeffrey D. P. Kenney

We present Gemini Near-infrared Integral Field Spectrograph (NIFS) observations of the inner $1.5\times1.5$ kpc$^2$ of the narrow-line Seyfert 1 galaxy Mrk 42 at a spatial resolution of 60 pc and spectral resolution of 40 km s$^{-1}$. The…

星系天体物理 · 物理学 2018-03-21 Moire G. Hennig , Rogemar A. Riffel , O. L. Dors , Rogerio Riffel , Thaisa Storchi-Bergmann , Luis Colina

The merger remnant NGC 34 is a local luminous infrared galaxy (LIRG) hosting a nuclear starburst and a hard X-ray source associated with a putative, obscured Seyfert~2 nucleus. In this work, we use adaptive optics assisted near infrared…

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

NGC 4527 is a nearby edge-on spiral galaxy with both starburst and AGN features, hosting a LINER nucleus. We present a radio study of the large-scale structure and nuclear region of this galaxy, based on new uGMRT observations at 700 and…

星系天体物理 · 物理学 2025-09-03 C. A. Galante , G. E. Romero , J. Saponara , P. Benaglia

We present our recent spectrophotometric results of the infrared luminous Seyfert 2 galaxy NGC 7679. We find compelling evidence of the presence of a recent nuclear starburst, revealed by the observations of a) the spectral features of high…

天体物理学 · 物理学 2009-11-06 Q. Gu , J. Huang , J. A. de Diego , D. Dultzin-Hacyan , S. Lei , E. Benitez

We present a study of the central 2.3 kpc of NGC 5135, a nearby Luminous Infrared Galaxy (LIRG) with an AGN and circumnuclear starburst. Our main results are based on intermediate spectral resolution (~ 3000-4000) near infrared data taken…

宇宙学与河外天体物理 · 物理学 2014-11-18 A. G. Bedregal , L. Colina , A. Alonso-Herrero , S. Arribas

We study the extended nuclear emission of the starburst galaxy NGC 1365. A weak obscured AGN and a strong starburst both contribute to the observed X-ray, optical, infrared, and radio emission in the inner 2kpc. The X-ray emission is…

高能天体物理现象 · 物理学 2009-03-10 I. V. Strateva , S. Komossa

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

High quality infrared spectra of active galaxies including the stellar absorption features of Si at 1.59 um, CO(6,3) at 1.62 um, and CO(2,0) at 2.29 um are used to measure the stellar mass to light ratio at 1.65 um (M_H/L) and investigate…

天体物理学 · 物理学 2007-05-23 E. Oliva , L. Origlia , R. Maiolino , A. F. M. Moorwood

Hidden from optical view in the starburst region of the dwarf galaxy NGC 5253 lies an intense radio source with an unusual spectrum which could be interpreted variously as nebular gas ionized by a young stellar cluster or nonthermal…

天体物理学 · 物理学 2009-11-06 Varoujan Gorjian , Jean L. Turner , Sara C. Beck

We present results from a 34 ks Chandra/ACIS-S observation of the nearby (d=3.1 Mpc) lenticular galaxy NGC 5102, previously shown to have an unusually low X-ray luminosity. We detect eleven X-ray point sources within the the $D_{25}$…

天体物理学 · 物理学 2009-11-11 R. P. Kraft , L. A. Nolan , T. J. Ponman , C. Jones , S. Raychaudhury

We report on the discovery of several compact regions of mid-infrared emission in the starforming circum nuclear disk of the starburst/Seyfert2 galaxy NGC7582. The compact sources do not have counterparts in the optical and near-infrared,…

天体物理学 · 物理学 2009-11-11 M. Wold , E. Galliano

We present observations of a massive star cluster near the nuclear region of the nearby starburst galaxy NGC 253. The peak of near-infrared emission, which is spatially separated by 4" from the kinematic center of the galaxy, is coincident…

太阳与恒星天体物理 · 物理学 2010-01-15 Katherine A. Kornei , Nate McCrady

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 new XMM-Newton observation of the Ultra Luminous Infrared Galaxy (ULIRG) NGC 6240. We analyze the reflecting grating spectrometer (RGS) data, and data from the other instruments, and find a starburst dominated 0.5-3 keV spectrum…

天体物理学 · 物理学 2009-11-11 Hagai Netzer , Doron Lemze , Shai Kaspi , I. M. George , T. J. Turner , D. Lutz , T. Boller , Doron Chelouche
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