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相关论文: Halpha rotation curves: the soft core question

200 篇论文

We study the structural properties of Low Surface Brightness galaxies (LSB) using a sample of 263 galaxies observed by the Green Bank Telescope (Schneider et al 1992). We perform 2D decompositions of these galaxies in the SDSS $g$, $r$ and…

星系天体物理 · 物理学 2018-05-16 Isha Pahwa , Kanak Saha

High-quality observations of dark matter-dominated low surface brightness (LSB) galaxies indicate that, in contrast to the triaxial, centrally-concentrated cuspy halos formed in collisionless simulations of halo assembly, these galaxies…

宇宙学与河外天体物理 · 物理学 2015-05-30 Rachel Kuzio de Naray , Kristine Spekkens

We present new Halpha+[NII] imaging data of late-type galaxies in the Herschel Reference Survey aimed at studying the star formation properties of a K-band-selected, volume-limited sample of nearby galaxies. The Halpha+[NII] data are…

星系天体物理 · 物理学 2015-07-08 A. Boselli , M. Fossati , G. Gavazzi , L. Ciesla , V. Buat , S. Boissier , T. Hughes

We present $UBVI$ and H$\alpha$ images of a sample of Low Surface Brightness (LSB) disk galaxies. These galaxies are generally late types, if they can be sensibly classified at all. However, they are not dwarfs, being intrinsically large…

天体物理学 · 物理学 2016-08-30 Stacy McGaugh , Jim Schombert , Greg Bothun

We investigate the effects of numerous dark matter subhalos in a galaxy-sized halo on the events of strong lensing, to assess their presence as expected from the cold dark matter scenario. Lens galaxies are represented by a smooth ellipsoid…

天体物理学 · 物理学 2009-11-07 Masashi Chiba

This paper presents surface photometry (B,V, I, J, H, K) and H_alpha rotation curves of 27 isolated spiral galaxies. The final goal is to obtain the mass distribution of a sample of isolated spiral galaxies in order to model their gas…

天体物理学 · 物理学 2009-11-11 I. Perez , I. Marquez , K. Freeman , R. Fux

While N-body simulations testify for a cuspy profile of the central region of the dark matter haloes, observations favor a shallow, cored density profile of the central region of, at least, some spiral galaxies and dwarf spheroidals. We…

高能天体物理现象 · 物理学 2014-07-15 Anton N. Baushev

We present the Fabry-Perot observations obtained for a new set of 108 galaxies that completes the GHASP survey (Gassendi HAlpha survey of SPirals). The GHASP survey consists of 3D Ha data cubes for 203 spiral and irregular galaxies,…

天体物理学 · 物理学 2009-11-13 B. Epinat , P. Amram , M. Marcelin , C. Balkowski , O. Daigle , O. Hernandez , L. Chemin , C. Carignan , J. -L. Gach , P. Balard

The thickness of the neutral hydrogen layer, coupled with the rotation curve, traces the outer dark matter potential. We estimate the amplitude of the flaring in spiral galaxies from a 3D model of the HI gas. Warps in particular are…

天体物理学 · 物理学 2007-05-23 J. -F. Becquaert , F. Combes

We present a systematic analysis of the rotation curves of 187 galaxies with masses greater than 10^10 M_sol, with atomic gas masses from the GALEX Arecibo Sloan Survey (GASS), and with follow-up long-slit spectroscopy from the MMT. Our…

星系天体物理 · 物理学 2015-08-06 Guinevere Kauffmann , Mei-ling Huang , Sean Moran , Timothy Heckman

We investigate the stellar disk properties of a sample of 19 nearby spiral galaxies with low inclination and late Hubble type (Scd or later). We combine our high-resolution HST I-band observations with existing ground-based optical images…

天体物理学 · 物理学 2009-11-07 Torsten Boeker , Rebecca Stanek , Roeland P. van der Marel

This project is the continuation of our study of faint Low Surface Brightness Galaxies (fLSBs) in one of the densest nearby galaxy regions known, the Coma cluster. Our goal is to improve our understanding of the nature of these objects by…

天体物理学 · 物理学 2009-11-13 C. Adami , R. Pello , M. P. Ulmer , J. C. Cuillandre , F. Durret , A. Mazure , J. P. Picat , R. Scheidegger

Stellar and gas kinematics of galaxies are a sensitive probe of the dark matter distribution in the halo. The popular fuzzy dark matter models predict the peculiar shape of density distribution in galaxies: specific dense core with sharp…

宇宙学与河外天体物理 · 物理学 2023-06-07 Mariia Khelashvili , Anton Rudakovskyi , Sabine Hossenfelder

In the previous papers in this series, we have measured the stellar and \hi content in a sample of edge-on galaxies. In the present paper, we perform a simultaneous rotation curve and vertical force field gradient decomposition for five of…

星系天体物理 · 物理学 2016-10-26 S. P. C. Peters , P. C. van der Kruit , R. J. Allen , K. C. Freeman

We present deep, high velocity resolution (~1.6 km/s) Giant Meterwave Radio Telescope (GMRT) HI 21cm synthesis images of the faint (M_B ~ -10.6) local group dwarf galaxy DDO210. We find that the HI distribution in the galaxy is not…

天体物理学 · 物理学 2009-11-10 Ayesha Begum , Jayaram N. Chengalur

We examine the circular velocity profiles of galaxies in {\Lambda}CDM cosmological hydrodynamical simulations from the EAGLE and LOCAL GROUPS projects and compare them with a compilation of observed rotation curves of galaxies spanning a…

I summarize some results from the recent CO survey of late-type, low surface brightness (LSB) spiral galaxies by Matthews et al. (2005). We have now detected CO emission from six late-type, LSB spirals, demonstrating that despite their…

天体物理学 · 物理学 2015-06-24 L. D. Matthews

We investigate the dynamics of starbursting dwarf galaxies, using both new and archival HI observations. We consider 18 nearby galaxies that have been resolved into single stars by HST observations, providing their star formation history…

星系天体物理 · 物理学 2014-06-23 Federico Lelli , Marc Verheijen , Filippo Fraternali

We analyze HST+WFPC2 images of 77 early-type galaxies. Brightness profiles are classed into "core" or "power-law" forms. Cores are typically rounder than power-law galaxies. Nearly all power-laws with central ellipticity >=0.3 have stellar…

We have used dedicated 0.7m telescopes in California and Israel to image the halos of ~200 galaxies in the Local Volume to 29 mag/sq arcsec, the sample mainly drawn from the 2MASS Large Galaxy Atlas (LGA). We supplement the LGA sample with…