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相关论文: NGC6240: Merger-Induced Star Formation & Gas Dynam…

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We report near-infrared integral field spectroscopy of the luminous merging galaxy NGC 6240. Stellar velocities show that the two K-band peaks separated by 1.6arcsec are the central parts of inclined, rotating disk galaxies with equal mass…

天体物理学 · 物理学 2009-10-31 M. Tecza , R. Genzel , L. J. Tacconi , S. Anders , L. E. Tacconi-Garman , N. Thatte

NGC6240 is a well-studied nearby galaxy system in the process of merging. Based on optical, X-ray, and radio observations, it is thought to harbor two active nuclei We carried out a detailed optical 3D spectroscopic study to investigate the…

星系天体物理 · 物理学 2020-01-15 W. Kollatschny , P. M. Weilbacher , M. W. Ochmann , D. Chelouche , A. Monreal-Ibero , R. Bacon , T. Contini

High resolution, 1.1, 1.6, and 2.2 micron imaging of the luminous infrared galaxy NGC 6090 obtained with NICMOS of the Hubble Space Telescope are presented. These new observations are centered on the two nuclei of the merger, and reveal the…

天体物理学 · 物理学 2009-10-31 N. Dinshaw , A. S. Evans , H. Epps , N. Z. Scoville , M. Rieke

We present preliminary results of an HST/NICMOS program to image merger remnants in the J, H and K bands. The nuclear brightness profiles for most sample galaxies are similar to those typical for elliptical galaxies, but some (including the…

天体物理学 · 物理学 2007-05-23 R. P. van der Marel , D. Zurek

We present high spatial resolution X-ray Chandra HRC and HST WFPC2 Halpha observations of the prototypical infrared luminous galaxy NGC6240. The central region of this system shows a remarkably complex morphology, with filaments and loops…

天体物理学 · 物理学 2009-11-07 P. Lira , M. J. Ward , A. Zezas , S. S. Murray

The role of major mergers in galaxy evolution is investigated through a detailed characterization of the stellar populations, ionized gas properties, and star formation rates (SFR) in the early-stage merger LIRGs IC 1623 W and NGC 6090, by…

We analyse new spatially resolved integral field spectroscopic H- and K-band data at a resolution of 0.3arcsec (100pc) and re-analyse interferometric CO(2-1) line observations of the prototypical merging system Arp220. We find that the…

宇宙学与河外天体物理 · 物理学 2015-05-27 H. Engel , R. I. Davies , R. Genzel , L. J. Tacconi , E. Sturm , D. Downes

We report adaptive optics H- and K-band spectroscopy of the inner few arcsec of the luminous merger/ULIRG/QSO Mkn231, at spatial resolutions as small as 0.085". For the first time we have been able to resolve the active star forming region…

天体物理学 · 物理学 2009-11-10 R. I. Davies , L. J. Tacconi , R. Genzel

We present deep CO observations of NGC6240 performed with the IRAM Plateau de Bure Interferometer (PdBI). NGC6240 is the prototypical example of a major galaxy merger in progress, caught at an early stage, with an extended,…

宇宙学与河外天体物理 · 物理学 2015-06-12 C. Feruglio , F. Fiore , R. Maiolino , E. Piconcelli , H. Aussel , D. Elbaz , E. Le Floc'h , E. Sturm , R. Davies , C. Cicone

We present star formation rates based on cold and ionized gas measurements of Mrk 266 (NGC 5256), a system composed of two colliding gas-rich galaxies, each hosting an active galactic nucleus. Using $^{12}$CO (1-0) observations with the…

We investigate the triggering mechanism and the structural properties of obscured luminous active galactic nuclei from a detailed study of the rest-frame $B$ and $I$ HST images of 29 nearby ($z\approx 0.04-0.4$) optically selected type 2…

星系天体物理 · 物理学 2019-06-05 Dongyao Zhao , Luis C. Ho , Yulin Zhao , Jinyi Shangguan , Minjin Kim

We present observations and dynamical models of the stellar nuclear clusters (NCs) at the centres of NGC 4244 and M33. We then compare these to an extensive set of simulations testing the importance of purely stellar dynamical mergers on…

宇宙学与河外天体物理 · 物理学 2015-05-27 Markus Hartmann , Victor P. Debattista , Anil Seth , Michelle Cappellari , Thomas R. Quinn

Galaxy mergers are central to our understanding of galaxy formation, especially within the context of hierarchical models. Besides having a large impact on the star formation history, mergers are also able to influence gas motions at the…

We present high-quality aperture synthesis observations of the neutral hydrogen distribution in a sample of five galactic systems believed to be involved in progressive stages of merging: Arp295, NGC4676, NGC520, NGC3921, and NGC7252. These…

天体物理学 · 物理学 2009-10-28 J. E. Hibbard , J. H. van Gorkom

Integral field spectroscopy in the K-band (1.9-2.4um) was performed on four IR-bright star clusters and the two nuclei in NGC 4038/4039 (``The Antennae''). Two of the clusters are located in the overlap region of the two galaxies, and…

We present a 3-dimensional data cube of the K band continuum and the Br-gamma, H2 S(0) and S(1) lines within the central 18.5" x 13.8" (520 pc x 390 pc) region of NGC 6946. Data were obtained using OSIRIS, a near-infrared Integral Field…

宇宙学与河外天体物理 · 物理学 2015-06-16 Chao-Wei Tsai , Jean L. Turner , Sara C. Beck , David S. Meier , Shelley A. Wright

We present new dynamical models of the merger remnant NGC 7252 which include star formation simulated according to various phenomenological rules. By using interactive software to match our model with the observed morphology and gas…

宇宙学与河外天体物理 · 物理学 2015-05-18 Li-Hsin Chien , Joshua Edward Barnes

Imaging of the Antennae galaxies (NGC 4038/4039) with the Infrared Array Camera (IRAC) aboard the Spitzer Space Telescope reveals large concentrations of star forming activity away from both nuclei of the two merging galaxies. These images…

NGC 6240 is a rare object in the local universe: an active merger remnant viewed at the point of merging where two active galactic nuclei are visible. We present IRAC data of this object, providing high sensitivity maps of the stellar and…

天体物理学 · 物理学 2009-11-13 Stephanie J. Bush , Zhong Wang , Margarita Karovska , Giovanni G. Fazio

To study the properties of the interstellar medium in the prototypical merging system of the Antennae galaxies (NGC 4038 and NGC 4039), we have obtained CO(1-0), (2-1) and (3-2) line maps, as well as a map of the 870 micron continuum…

天体物理学 · 物理学 2009-11-13 A. Schulz , C. Henkel , D. Muders , R. Q. Mao , M. Roellig , R. Mauersberger
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