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相关论文: The kinematics of the diffuse ionized gas in NGC 4…

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A detailed kinematic analysis of ionized gas in the nearby irregular galaxy NGC 4449 is presented. Observations are conducted in the spectral lines of Halpha and [SII]. Our scanning Fabry--Perot interferometric observations are presented…

To better understand diffuse ionized gas kinematics and halo rotation in spiral galaxies, we have developed a model in which clouds are ejected from the disk and follow ballistic trajectories through the halo. The behavior of clouds in this…

天体物理学 · 物理学 2009-11-07 J. A. Collins , R. A. Benjamin , R. J. Rand

Existing long-slit spectral data for edge-on spiral galaxies suggesting that their Diffuse Ionized Gas (DIG) halos rotate slower than their underlying disks are summarized. An attempt to characterize lagging halos using a model of purely…

天体物理学 · 物理学 2007-05-23 R. J. Rand

The structure and kinematics of gaseous, disk-halo interfaces are imprinted with the processes that transfer mass, metals, and energy between galactic disks and their environments. We study the extraplanar diffuse ionized gas (eDIG) layer…

星系天体物理 · 物理学 2020-01-08 Erin Boettcher , John S. Gallagher , Ellen G. Zweibel

Abridged. Context. The metal content of dwarf galaxies and the metal enrichment of the intergalactic medium both suggest that mass loss from galaxies is a significant factor for the chemical evolution history of galaxies, in particular of…

天体物理学 · 物理学 2009-11-13 J. van Eymeren , M. Marcelin , B. Koribalski , R. -J. Dettmar , D. J. Bomans , J. -L. Gach , P. Balard

We present a multiphase, resolved study of the galactic wind extending from the nearby starburst galaxy NGC 4666. For this we use VLT/MUSE observations from the GECKOS program and HI data from the WALLABY survey. We identify both ionised…

We present key results from deep spectra of the Diffuse Ionized Gas (DIG) halo of the edge-on galaxy NGC 5775. [NII]6583 has been detected up to about z=13 kpc above the plane in one of two vertically oriented long slits -- making this the…

天体物理学 · 物理学 2009-10-31 Richard J. Rand

We study two dimensional Fabry-Perot interferometric observations of the nearby face-on late-type spiral galaxy, NGC 628, in order to analyse the ionized gas component of the interstellar medium. Covering the galaxy out to a radius larger…

In order to understand the formation and evolution of dIm galaxies, one needs to understand their three-dimensional structure. We present measurements of the stellar velocity dispersion in NGC 1569, a nearby post-starburst dIm galaxy. The…

宇宙学与河外天体物理 · 物理学 2013-04-03 Megan Johnson , Deidre A. Hunter , Se-Heon Oh , Hong-Xin Zhang , Bruce Elmegreen , Elias Brinks , Erik Tollerud , Kimberly Herrmann

In this letter we present first results from spectroscopic observations of Diffuse Ionized Gas (DIG) in the halo of NGC5775 obtained with FORS1 attached to UT1/Antu of the Very Large Telescope (VLT). At our slit position perpendicular to…

天体物理学 · 物理学 2007-05-23 R. Tuellmann , R. -J. Dettmar , M. Soida , M. Urbanik , J. Rossa

We present a study of the kinematics of the ionised gas in the nearby spiral galaxy NGC 2403 using deep long-slit spectra obtained with the 4.2-m William Herschel Telescope. The data show the presence of a halo component of ionised gas that…

天体物理学 · 物理学 2009-11-10 Filippo Fraternali , Tom Oosterloo , Renzo Sancisi

We present high and moderate spectral resolution spectroscopy of diffuse ionized gas (DIG) emission in the halo of NGC 891. The data were obtained with the SparsePak integral field unit at the WIYN Observatory. The wavelength coverage…

天体物理学 · 物理学 2011-02-11 George H. Heald , Richard J. Rand , Robert A. Benjamin , Matthew A. Bershady

In this third paper of a series, we study the kinematics of the ionised gas and stars, calculating the dynamical masses of the circumnuclear star-forming regions in the ring of of the face-on spiral NGC 7742. We have used high spectral…

星系天体物理 · 物理学 2025-04-02 S. Zamora , A. I. Díaz , Roberto Terlevich , Elena Terlevich , R. Amorín

Gaseous, disk-halo interfaces are shaped by processes that are critical to galaxy evolution, including gas accretion and outflows. Extraplanar diffuse ionized gas (eDIG) layers are characterized by scale heights that largely exceed those…

星系天体物理 · 物理学 2025-07-01 Hanjue Zhu , Erin Boettcher , Hsiao-Wen Chen

As part of a large study to map the distribution of star formation across galactic disks, we have obtained deep Halpha images of the nearby Sculptor Group spirals NGC 247 and NGC 7793. These images are of sufficiently high quality that they…

天体物理学 · 物理学 2007-05-23 Annette M. N. Ferguson , Rosemary F. G. Wyse , J. S. Gallagher , Deidre A. Hunter

Abridged. The feedback between massive stars and the interstellar medium is one of the most important processes in the evolution of dwarf galaxies. This interaction results in numerous neutral and ionised gas structures that have been found…

宇宙学与河外天体物理 · 物理学 2017-08-30 J. van Eymeren , B. S. Koribalski , A. R. Lopez-Sanchez , R. -J. Dettmar , D. J. Bomans

The diffuse ionized gas (DIG) is an important component of the interstellar medium that can provide insights into the different physical processes affecting the gas in galaxies. We utilise optical IFU observations of 71 gas-stripped and…

In order to examine the excitation and ionization mechanism of extraplanar diffuse ionized gas (DIG) we have obtained optical longslit spectra of seven edge-on spiral galaxies. In four objects the brightest emission lines can be traced out…

天体物理学 · 物理学 2007-05-23 R. Tuellmann , R. -J. Dettmar

We present the kinematics and photometry of the stars and of the ionized gas near the centre of the S0 galaxy NGC4036. Dynamical models based on the Jeans Equation have been constructed from the stellar data to determine the gravitational…

天体物理学 · 物理学 2009-10-31 P. Cinzano , H. -W. Rix , M. Sarzi , E. M. Corsini , W. W. Zeilinger , F. Bertola

We analyze the magnetic field geometry and the transport processes of the cosmic rays of the edge-on spiral starburst galaxy NGC 4666 from CHANG-ES radio continuum data in two frequencies; 6 GHz (C-band) and 1.5 GHz (L-band). Supplementary…

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