2,982 datasets found

Keywords: radial velocity

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  • Upper Scorpius and Ophiuchus members

    Understanding how star formation begins and propagates through molecular clouds is a fundamental but still open question. One major difficulty in addressing this question is the...
  • ATLAS3D project. III.

    We provide a census of the apparent stellar angular momentum within one effective radius of a volume-limited sample of 260 early-type galaxies (ETGs) in the nearby Universe,...
  • Multiwavelength study of RX J1117.4+0743

    We present a multiwavelength study of the poor cluster RX J1117.4+0743 ([VMF98] 097) at z=0.485, based on GMOS/Gemini South g' and r' photometry and spectroscopy, and XMM-Newton...
  • Radial velocities of Leo I stars

    We present a wide-field (4.5deg^2^) photometric and spectroscopic survey of the Leo I dwarf spheroidal (dSph) galaxy to explore its extended morphology and dynamics. To select...
  • Hypervelocity stars. II.

    Hypervelocity stars (HVSs) are stars ejected completely out of the Milky Way by three-body interactions with the massive black hole in the Galactic center. We describe 643 new...
  • Satellites orbiting isolated galaxies

    Using the Sloan Digital Sky Survey (SDSS), we probe the halo mass distribution by studying the velocities of satellites orbiting isolated galaxies. In a subsample that covers...
  • Velocities of blue stars near (l,b)=(198,-27)

    We present evidence for a ring of stars in the plane of the Milky Way, extending at least from l=180{deg} to 227{deg} with turnoff magnitude g~19.5; the ring could encircle the...
  • New PN in southern Galactic Bulge

    We present the results of a deep and uniform narrowband H{alpha} imaging survey for planetary nebulae (PNs) in the southern Galactic bulge. In our survey, we have found 56 new...
  • Radial velocities for the HD 3167 system

    HD 3167 is a bright (V=8.9), nearby K0 star observed by the NASA K2 mission (EPIC 220383386), hosting two small, short-period transiting planets. Here we present the results of...
  • Radial velocities in UGC 842 and NGC 6034

    We present a new insight on NGC 6034 and UGC 842, two groups of galaxies previously reported in the literature as being fossil groups. The study is based on optical photometry...
  • MCG pairs and triples of galaxies

    We derive the number of dynamically close companions per galaxy (N_c_) and their total luminosity (L_c_) for galaxies in the Millennium Galaxy Catalogue (MGC, 2003, Cat. ). N_c_...
  • Members of the Sculptor dwarf spheroidal galaxy

    The results of a wide-field survey of the Sculptor dwarf spheroidal galaxy are presented. Our aims were to obtain an accurate map of the outer structure of Sculptor and to...
  • Photometry in the NGC 4756 group of galaxies

    This paper is part of a series that focuses on investigating galaxy formation and evolution in small-scale systems of galaxies in low-density environments. We present results...
  • The UZC-SSRS2 group catalog

    We apply a friends-of-friends algorithm to the combined Updated Zwicky Catalog (UZC, Cat. )and Southern Sky Redshift Survey (SSRS2, Cat. ) to construct a catalog of 1168 groups...
  • Kinematic Profiles of S0 Galaxies

    Stellar rotation curves, velocity dispersion profiles, and line of sight velocity distributions (LOSVD) as derived from absorption-lines are presented for the major axes of 18...
  • The survival of Sagittarius dwarf galaxy

    The Sagittarius dwarf spheroidal galaxy, the closest satellite galaxy of the Milky Way, has survived for many orbits about the Galaxy. Extent numerical calculations modeled this...
  • Tully-Fisher Relation. I.

    Observational parameters which can be used for redshift-independent distance determination using the Tully-Fisher (TF) technique are given for 782 spiral galaxies in the fields...
  • Velocities in Abell 3266

    We present 387 velocities covering an area 1.8x1.8{deg}^2^, including 229 new galaxy velocities obtained from 309 spectra, of which 317 appear to be cluster members according to...
  • TESS, CHEOPS and ESPRESSO data of HD 22946

    Multi-planet systems are important sources of information regarding the evolution of planets. However, the long-period planets in these systems often escape detection. These...
  • A CHEOPS-enhanced view of the HD3167 system

    Much remains to be understood about the nature of exoplanets smaller than Neptune, most of which have been discovered in compact multi-planet systems. With its inner ultra-short...
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