Results 11 to 20 of about 77,155 (253)
Production of Milky Way structure by the Magellanic Clouds [PDF]
Previous attempts at disturbing the galactic disk by the Magellanic Clouds relied on direct tidal forcing. However, by allowing the halo to actively respond rather than remain a rigid contributor to the rotation curve, the Clouds may produce a wake in the halo which then distorts the disk.
Hernquist L.+5 more
arxiv +6 more sources
Modelling dust extinction in the Magellanic Clouds [PDF]
We model the extinction profiles observed in the Small and Large Magellanic clouds with a synthetic population of dust grains consisting by core-mantle particles and a collection of free-flying polycyclic aromatic hydrocarbons.
Aresu, Giambattista+4 more
core +6 more sources
THE MAGELLANIC CLOUDS. XV. ON THE TILT OF THE LARGE CLOUD. [PDF]
Nail VM, Shapley H.
europepmc +3 more sources
MAGELLANIC CLOUDS. XIII. COMPARISON OF MAGELLANIC AND GALACTIC ECLIPSING VARIABLES. [PDF]
Russell HN.
europepmc +2 more sources
Molecules in the Magellanic Clouds [PDF]
In this short review we describe recent new observations of millimetre transitions of molecules in selected regions of the Magellanic Clouds. The observations were made using the Swedish-ESO Submillimetre Telescope, SEST, (Booth et al. 1989), the relatively high resolution of which facilitates, for the first time, observations of individual giant ...
T Degraauw, Rs Booth
openaire +3 more sources
Discovery of the Magellanic Stellar Stream Out to 100 kpc
The Magellanic Stream (MS)—an enormous ribbon of gas spanning 140° of the southern sky trailing the Magellanic Clouds—has been exquisitely mapped in the five decades since its discovery.
Vedant Chandra+9 more
doaj +1 more source
CCD imagers for the Transiting Exoplanet Survey Satellite from benchtop to space environment
Abstract The Transiting Exoplanet Survey Satellite (TESS) is a Massachusetts Institute of Technology‐led NASA Explorer‐class mission planned to spend 2 years discovering transiting exoplanets by an all‐sky survey. The observatory contains four wide field‐of‐view camera systems for a total of 16.8 Megapixel, low‐noise, low‐power CCD detectors.
Vyshnavi Suntharalingam+5 more
wiley +1 more source
Cepheids in the Magellanic Clouds [PDF]
AbstractIn the past few years, the Magellanic Clouds have been the targets for several major variable star surveys. The results of these surveys are now becoming available and it is clear that a Renaissance in LMC and SMC variable star research will result.
P. J. Quinn+14 more
openaire +3 more sources
Magellanic Clouds Cepheids: Thorium Abundances [PDF]
The analysis of the high-resolution spectra of 31 Magellanic Clouds Cepheid variables enabled the identification of thorium lines. The abundances of thorium were found with spectrum synthesis method. The calculated thorium abundances exhibit correlations
Yeuncheol Jeong+5 more
doaj +1 more source
LRO‐LAMP Lunar South Pole Cold Traps: Assessment of H2O and Potential CO2 and NH3 Reserves
Abstract Nighttime Lyman Alpha Mapping Project (LAMP) observations are used to investigate condensed volatiles at the south polar region of the Moon. This study incorporates LAMP data from the first ∼7 years of the mission and Diviner annual maximum temperatures to search for volatile signatures associated with H2O, NH3, and CO2. Other stable potential
L. O. Magaña+15 more
wiley +1 more source