Results 101 to 110 of about 34,432 (305)
Dwarf Spheroidal Galaxies in the M101 Group and Behind it [PDF]
Astrophysics, 2019 published in Astrophysics, v.62, p.293 ...
Karachentsev, I. D., Makarova, L. N.
openaire +2 more sources
PROTEOMICS, Volume 24, Issue 12-13, June 2024.Abstract MALDI mass spectrometry imaging (MALDI imaging) uniquely advances cancer research, by measuring spatial distribution of endogenous and exogenous molecules directly from tissue sections. These molecular maps provide valuable insights into basic and translational cancer research, including tumor biology, tumor microenvironment, biomarker ...
Maren Nicole Stillger +4 more
wiley +1 more source
Are Nuclear Star Clusters the Precursors of Massive Black Holes?
Advances in Astronomy, Volume 2012, Issue 1, 2012., 2012 We present new upper limits for black hole masses in extremely late type spiral galaxies. We confirm that this class of galaxies has black holes with masses less than 106M⊙, if any. We also derive new upper limits for nuclear star cluster masses in massive galaxies with previously determined black hole masses.
Nadine Neumayer +2 more
wiley +1 more source
HI Observations Towards the Sagittarius Dwarf Spheroidal Galaxy [PDF]
, 1999 We have measured the 21-cm line of Galactic HI over more than 50 square degrees in the direction of the Sagittarius dwarf spheroidal galaxy. The data show no evidence of HI associated with the dwarf spheroidal which might be consider analogous to the ...
Burton, W. B., Lockman, Felix J.
core +2 more sources
Whiting 1: Confirmation of its accretion by the Milky Way
EPJ Web of Conferences, 2017 We investigate the association of Whiting 1 with the Sagittarius tidal stream by obtaining radial velocities for a sample of 101 stars observed with VIMOS.
Carballo-Bello Julio A. +6 more
doaj +1 more source
Chemical compositions of six metal-poor stars in the ultra-faint dwarf spheroidal galaxy Boötes I [PDF]
, 2014 Context. Ultra-faint dwarf galaxies recently discovered around the Milky Way (MW) contain extremely metal-poor stars, and might represent the building blocks of low-metallicity components of the MW.
M. Ishigaki +3 more
semanticscholar +1 more source
Updated Bounds on Axion‐Like Particle Dark Matter with the Optical MUSE‐Faint Survey
Annalen der Physik, Volume 536, Issue 1, January 2024.This study presents bounds on the axion‐like particle (ALP) to two‐photon coupling in the mass range $2.65‐5.27$ eV. The signal from ALP decay are sought in the Multi Unit Spectroscopic Explorer (MUSE) observations of five dwarf spheroidal galaxies, under the assumption that ALPs make up the whole dark matter.
Elisa Todarello
wiley +1 more source
Pulsar‐Driven Jets in Supernovae, Gamma‐Ray Bursts, and the Universe
Advances in Astronomy, Volume 2012, Issue 1, 2012., 2012 The bipolarity of Supernova 1987A can be understood through its very early light curve from the CTIO 0.4 m telescope and IUE FES and following speckle observations of the “Mystery Spot”. These indicate a beam/jet of light/particles, with initial collimation factors >104 and velocities >0.95 c, involving up to 10−5 M⊙ interacting with circumstellar ...
John Middleditch +1 more
wiley +1 more source
, 2019 In this work we use structural properties of Milky Way's outer halo ($R_G > 25\,\mathrm{kpc}$) satellites (dwarf spheroidal galaxies, ultra-faint dwarf galaxies and globular clusters) derived from deep, wide-field and homogeneous data, to present ...
Carballo-Bello, Julio A. +8 more
core +1 more source
About the morphology of dwarf spheroidal galaxies and their dark matter content [PDF]
, 2003 The morphological properties of the Carina, Sculptor and Fornax dwarfs are investigated using new wide field data with a total area of 29 square degrees.
Burkert, A. +3 more
core +3 more sources