Results 111 to 120 of about 579,982 (342)
Molecular Gas in Elliptical Galaxies: Distribution and Kinematics
, 2002 I present interferometric images (approx. 7" resolution) of CO emission in five elliptical galaxies and nondetections in two others. These data double the number of elliptical galaxies whose CO emission has been fully mapped.
Braine J. +12 more
core +2 more sources
Late-type galaxies observed with SAURON. Two-dimensional stellar and emission-line kinematics of 18 spirals [PDF]
, 2005 We present the stellar and gas kinematics of a sample of 18 nearby late-type spiral galaxies (Hubble types ranging from Sb to Sd), observed with the integral-field spectrograph SAURON at the 4.2-m William Herschel Telescope.
Andersen, DR +9 more
core +2 more sources
Stellar 3D kinematics in the Draco dwarf spheroidal galaxy [PDF]
Astronomy & Astrophysics, 2019 Aims. We present the first three-dimensional internal motions for individual stars in the Draco dwarf spheroidal galaxy. Methods. By combining first-epoch Hubble Space Telescope observations and second-epoch Gaia Data Release 2 positions, we measured the
D. Massari +5 more
semanticscholar +1 more source
The Kinematics of Galactic Stellar Disks
Monthly Notices of the Royal Astronomical Society, 1998 11 pages, LaTeX (including 7 figures), uses paspconf.sty and epsf.sty, to be published in Proceedings of the EC Summer School on 'Astrophysical Discs', eds J. A. Sellwood and J.
Merrifield, M. R., Kuijken, K.
openaire +3 more sources
Advanced Functional Materials, EarlyView.Flexible piezoresistive pressure sensors underpin wearable and soft electronics. This review links sensing physics, including contact resistance modulation, quantum tunneling and percolation, to unified materials/structure design. We highlight composite and graded architectures, interfacial/porous engineering, and microstructured 3D conductive networks
Feng Luo +2 more
wiley +1 more source
The Astrophysical Journal, 2023 NGC 1052-DF4 was found to be the second “galaxy lacking dark matter” in the NGC 1052 group, based on its velocity dispersion of ${\sigma }_{\mathrm{gc}}={4.2}_{-2.2}^{+4.4}$ km s ^−1 as measured from the radial velocities of seven of its globular ...
Zili Shen +2 more
doaj +1 more source
Nuclear angular momentum of early-type galaxies hosting nuclear star clusters
, 2019 Nucleation is a common phenomenon in all types of galaxies and at least 70% of them host nuclear star clusters (NSCs) in their centres. Many of the NSCs co-habit with super-massive black holes and follow similar scaling relations with host galaxy ...
Lyubenova, Mariya, Tsatsi, Athanassia
core +1 more source
Large-Scale Model of the Milky Way: Stellar Kinematics and Microlensing Event Timescale Distribution in the Galactic Bulge [PDF]
, 2003 We build a stellar-dynamical model of the Milky Way barred bulge and disk, using a newly implemented adaptive particle method. The underlying mass model has been previously shown to match the Galactic near-infrared surface brightness as well as gas ...
Bissantz, Nicolai +2 more
core +3 more sources
Kinematical signatures of hidden stellar discs [PDF]
Monthly Notices of the Royal Astronomical Society, 1999 7 pages, 7 figures, uses mn ...
openaire +2 more sources
Advanced Functional Materials, EarlyView.ABSTRACT Traditional wearable exoskeletons rely on rigid structures, which limit comfort, flexibility, and everyday usability. This work introduces the fundamental technologies to create the first soft, lightweight, intelligent textile‐based exoskeletons (Texoskeletons) built using 1D sensors and actuators.
Amy Lukomiak +19 more
wiley +1 more source