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Related papers: Large stellar disks in small elliptical galaxies

200 papers

Nearly 400 Tycho-2 stars have been observed in a 720 square degree field in the direction of the North Galactic Pole with the high resolution echelle spectrograph ELODIE. Absolute magnitudes, effective temperatures, gravities and…

Astrophysics · Physics 2009-11-07 C. Soubiran , O. Bienaymé , A. Siebert

Recent progress is summarized on the determination of the density distributions of stars and dark matter, stellar kinematics, and stellar population properties, in the extended, low surface brightness halo regions of elliptical galaxies.…

Astrophysics of Galaxies · Physics 2015-05-20 Ortwin Gerhard

Ionized gas and stellar kinematical parameters have been measured along the major axis of 20 nearby disc galaxies. We discuss the properties of each sample galaxy distinguishing between those characterized by regular or peculiar kinematics.…

We have used the EFAR sample of galaxies to study the light distributions of early-type galaxies. We decompose the 2D light distribution of the galaxies in a flattened spheroidal component with a Sersic radial light profile and an inclined…

Using a large sample of galaxies from the SDSS-DR7, we have analysed the alignment of disk galaxies around cosmic voids. We have constructed a complete sample of cosmic voids (devoid of galaxies brighter than M_r-5 log(h) =-20.17) with…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Jesús Varela , Juan Betancort-Rijo , Ignacio Trujillo , Elena Ricciardelli

The most massive elliptical galaxies have low-density centers or cores that differ dramatically from the high-density centers of less massive ellipticals and bulges of disk galaxies. These cores have been interpreted as the result of…

Astrophysics of Galaxies · Physics 2015-06-17 J. Thomas , R. P. Saglia , R. Bender , P. Erwin , M. Fabricius

We have performed intermediate-resolution VLT/FORS spectroscopy and HST/ACS imaging of 129 field spiral galaxies within the FORS Deep Field. The galaxies cover the redshift range 0.1 < z < 1.0 and comprise all types from Sa to Sdm/Im.…

Astrophysics · Physics 2007-05-23 Asmus Boehm , Bodo L. Ziegler

We present collisionless simulations of dry mergers in groups of three to twenty-five galaxies to test the hypothesis that elliptical galaxies form at the centers of such groups. Mock observations of the central remnants confirm their…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 Dan S. Taranu , John Dubinski , H. K. C. Yee

We present spatially resolved stellar rotation velocity and velocity dispersion profiles form Keck/LRIS absorption-line spectra for 25 galaxies, mostly visually classified ellipticals, in three clusters at z=0.5. We interpret the…

Astrophysics · Physics 2009-11-11 Roeland P. van der Marel , Pieter G. van Dokkum

Using a high resolution hydrodynamical cosmological simulation of the formation of a massive spheroidal galaxy we show that elliptical galaxies can be very compact and massive at high redshift in agreement with recent observations.…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-11 Thorsten Naab , Peter H. Johansson , Jeremiah P. Ostriker

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…

Astrophysics · Physics 2009-11-13 Peter Yoachim , Julianne J. Dalcanton

The disks of spiral galaxies are generally elliptical rather than circular. The distribution of ellipticities can be fit with a log-normal distribution. For a sample of 12,764 galaxies from the Sloan Digital Sky Survey Data Release 1 (SDSS…

Astrophysics · Physics 2009-11-10 Barbara S. Ryden

We study massive disk galaxies (total stellar mass$>=10^{11}$ $\mathrm{M_{\odot}}$) from IllustrisTNG50 simulation, and perform 2-D structural decomposition of the galaxies using their idealised, synthetic SDSS images for z=0. We find an…

Astrophysics of Galaxies · Physics 2026-02-11 Suchira Sarkar , Kanak Saha

Mergers in the local universe present a unique opportunity for studying the transformations of galaxies in detail. Presented here are recent results, based on multi-wavelength, high-resolution imaging and medium resolution spectroscopy,…

Cosmology and Nongalactic Astrophysics · Physics 2010-05-12 Barry Rothberg , Jacqueline Fischer

We report high quality near-infrared spectroscopy of 12 ultra-luminous infrared galaxy mergers (ULIRGs). Our new VLT and Keck data provide ~0.5" resolution, stellar and gas kinematics of these galaxies most of which are compact systems in…

Astrophysics · Physics 2009-11-06 R. Genzel , L. J. Tacconi , D. Rigopoulou , D. Lutz , M. Tecza

We describe the evolution of hot interstellar gas in a family of low luminosity elliptical galaxies all having $M_B = -20$ but with different degrees of flattening (E0, E2, and E6) caused by rotation. The interstellar gas is furnished by…

Astrophysics · Physics 2009-10-30 Fabrizio Brighenti , William G. Mathews

Recent deep Hubble Space Telescope WFC3 imaging suggests that a majority of compact quiescent massive galaxies at z~2 may contain disks. To investigate this claim, we have compared the ellipticity distribution of 31 carefully selected…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 M. Chevance , A. Weijmans , I. Damjanov , R. G. Abraham , L. Simard , S. van den Bergh , E. Caris , K. Glazebrook

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…

Astrophysics · Physics 2009-11-07 Michiel Kregel , Pieter C. van der Kruit , Richard de Grijs

We have measured the intrinsic disk ellipticity for 7 nearby, nearly face-on spiral galaxies by combining Densepak integral-field spectroscopy with I-band imaging from the WIYN telescope. Initially assuming an axisymmetric model, we…

We present new kinematic measurements and modeling of a sample of 116 young stars in the central parsec of the Galaxy in order to investigate the properties of the young stellar disk. The measurements were derived from a combination of…

Astrophysics of Galaxies · Physics 2014-03-05 Sylvana Yelda , Andrea M. Ghez , Jessica R. Lu , Tuan Do , Leo Meyer , Mark R. Morris , Keith Matthews