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We report the identification of a super-thin disk (h_z~60 pc) in the edge-on spiral galaxy NGC 891. This component is only apparent after we perform a physically motivated attenuation correction, based on detailed radiation transfer models,…

宇宙学与河外天体物理 · 物理学 2013-09-05 Andrew Schechtman-Rook , Matthew A. Bershady

We probe the disk structure of the nearby, massive, edge-on spiral galaxy NGC 891 with sub-arcsecond resolution JHKs-band images covering ~+/-10 kpc in radius and +/-5 kpc in height. We measure intrinsic surface brightness profiles using…

宇宙学与河外天体物理 · 物理学 2013-07-26 Andrew Schechtman-Rook , Matthew A. Bershady

We present kinematic measurements of the thick and thin disks in two edge-on galaxies. We have derived stellar rotation curves at and above the galaxies' midplanes using Ca II triplet features measured with the GMOS spectrograph on Gemini…

天体物理学 · 物理学 2009-11-10 Peter Yoachim , Julianne J. Dalcanton

Disc truncations are the closest feature to an edge that galaxies have, but the nature of this phenomena is not yet understood. In this paper, we explore the truncations in two nearby (D ~15 Mpc) Milky Way-like galaxies: NGC 4565 and NGC…

星系天体物理 · 物理学 2018-11-16 Cristina Martinez-Lombilla , Ignacio Trujillo , Johan H. Knapen

`Superthins' are a subset of edge-on spiral galaxies exhibiting disks with large axial ratios (a/b>10), extraordinarily small stellar scale heights, and no bulge component. These are thus examples of dynamically cold, pure disk galaxies. We…

天体物理学 · 物理学 2007-05-23 L. D. Matthews , W. van Driel , J. S. Gallagher

We present I-band photometry, long-slit optical spectroscopy, and new aperture synthesis HI observations for eight late-type spirals with rotation velocities in the range 243 km/s < V_{rot} < 308 km/s. The sample will be used to study the…

天体物理学 · 物理学 2008-11-26 K. Spekkens , R. Giovanelli

(Abridged) We analyze the evolution of 42 spiral galaxies in the Spitzer Infrared Nearby Galaxies Survey, using extinction-corrected UV, optical and near-infrared radial profiles to probe the emission of stars of different ages as a…

宇宙学与河外天体物理 · 物理学 2015-05-27 J. C. Muñoz-Mateos , S. Boissier , A. Gil de Paz , J. Zamorano , R. C. Kennicutt , J. Moustakas , N. Prantzos , J. Gallego

We present an analysis of the H2 emission-line gas kinematics in the inner < 4 arcsec radius of six nearby spiral galaxies, based on AO-assisted integral-field observations obtained in the K-band with SINFONI/VLT. Four of the six galaxies…

星系天体物理 · 物理学 2015-06-18 X. Mazzalay , W. Maciejewski , P. Erwin , R. P. Saglia , R. Bender , M. H. Fabricius , N. Nowak , S. P. Rusli , J. Thomas

The stellar disc kinematics in a sample of fifteen intermediate- to late-type edge-on spiral galaxies are studied using a dynamical modeling technique. The sample covers a substantial range in maximum rotation velocity and deprojected…

天体物理学 · 物理学 2009-11-10 M. Kregel , P. C. van der Kruit

We consider seven distant galaxies with clearly evident spiral structure from HST images. Three of these were chosen from Vogt et al. (1996) (VFP) and have measured rotational velocities. Five were chosen from the Medium Deep Survey and are…

天体物理学 · 物理学 2009-10-30 A. C. Quillen , V. L. Sarajedini

Breaks in the radial luminosity profiles of galaxies have been until now mostly studied averaged over discs. Here we study separately breaks in thin and thick discs in 70 edge-on galaxies using imaging from the Spitzer Survey of Stellar…

We use the rotation curves of more than 100 disk galaxies to examine whether the structure of their surrounding dark halos is consistent with the universal density profile proposed by Navarro, Frenk & White (NFW profiles). Rotation curve…

天体物理学 · 物理学 2007-05-23 Julio F. Navarro

We present K'(2.1 micron) observations of four nearby flocculent spirals, which clearly show low-level spiral structure and suggest that kiloparsec-scale spiral structure is more prevalent in flocculent spirals than previously supposed. In…

天体物理学 · 物理学 2009-10-28 Michele D. Thornley

Superthin galaxies are a class of bulgeless, low surface brightness galaxies with strikingly high values of planar-to-vertical axes ratio $\rm(b/a> 10 - 20)$, possibly indicating the presence of an ultra-cold stellar disc. Using the…

星系天体物理 · 物理学 2021-01-29 K. Aditya , Arunima Banerjee

We present kinematic measurements of thin and thick disk components in a sample of nine edge-on galaxies. We extract stellar and ionized gas rotation curves at and above the galaxies' midplanes using the Ca II triplet absorption features…

天体物理学 · 物理学 2009-11-13 Peter Yoachim , Julianne J. Dalcanton

We present the results of a kinematic study of planetary nebulae in the extreme outskirts of two spiral galaxies, M83 (NGC 5236) and M94 (NGC 4736). We find that in the inner regions of the galaxies, the vertical velocity dispersion…

宇宙学与河外天体物理 · 物理学 2009-02-17 Kimberly A. Herrmann , Robin Ciardullo , Steinn Sigurdsson

We analyze the global structure of 34 late-type, edge-on, undisturbed, disk galaxies spanning a wide range of mass. We measure structural parameters for the galaxies using two-dimensional least-squares fitting to our $R$-band photometry.…

天体物理学 · 物理学 2008-11-26 Peter Yoachim , Julianne J. Dalcanton

We present rotation curves for 19, mostly luminous, early-type disk galaxies. Rotation velocities are measured from a combination of HI velocity fields and long-slit optical emission line spectra along the major axis. We find that the…

天体物理学 · 物理学 2008-11-26 E. Noordermeer , J. M. van der Hulst , R. Sancisi , R. S. Swaters , T. S. van Albada

We analyse the global structure of the old stellar discs in 34 edge-on spiral galaxies. The radial and vertical exponential scale parameters of the discs are obtained by applying an improved two-dimensional decomposition technique to our…

天体物理学 · 物理学 2009-11-07 Michiel Kregel , Pieter C. van der Kruit , Richard de Grijs

We present interferometric observations resolving the CO emission in the four gas-rich lenticular galaxies NGC 3032, NGC 4150, NGC 4459, and NGC 4526, and we compare the CO distribution and kinematics to those of the stars and ionized gas.…

天体物理学 · 物理学 2009-11-13 Lisa M. Young , Martin Bureau , Michele Cappellari
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