Results 11 to 20 of about 13,924,091 (398)

Development in astronomy and space science in Africa [PDF]

open access: yesNature Astronomy, 2018
The development of astronomy and space science in Africa has grown significantly over the past few years. These advancements make the United Nations Sustainable Development Goals more achievable, and open up the possibility of new beneficial ...
M. Pović   +22 more
semanticscholar   +3 more sources

Report on the Twelfth United Nations/European Space Agency Workshop on Basic Space Science [PDF]

open access: yesAstrophysics and Space Science 305(2006)325-330, 2006
Pursuant to recommendations of the United Nations Conference on the Exploration and Peaceful Uses of Outer Space (UNISPACE III) and deliberations of the United Nations Committee on the Peaceful Uses of Outer Space (UNCOPUOS), annual UN/European Space Agency workshops on basic space science have been held around the world since 1991.
Haubold, H. J., Wamsteker, W.
arxiv   +3 more sources

Predictions for ASKAP neutral hydrogen surveys [PDF]

open access: yes, 2012
The Australian Square Kilometre Array Pathfinder (ASKAP) will revolutionize our knowledge of gas-rich galaxies in the Universe. Here we present predictions for two proposed extragalactic ASKAP neutral hydrogen (H I) emission-line surveys, based on semi ...
A. Duffy   +16 more
semanticscholar   +1 more source

FOSSIL EVIDENCE FOR THE TWO-PHASE FORMATION OF ELLIPTICAL GALAXIES [PDF]

open access: yesAstrophysical Journal, 2013
Massive early-type galaxies (ETGs) have undergone dramatic structural evolution over the last 10 Gyr. A companion paper shows that nearby elliptical galaxies with M* ⩾ 1.3 × 1011M☉ generically contain three photometric subcomponents: a compact inner ...
Song Huang   +17 more
semanticscholar   +1 more source

A systematic survey for infrared star clusters with |b| < 20° using 2MASS [PDF]

open access: yes, 2006
We used star density maps obtained from the Two-Micron All-Sky Survey (2MASS) to obtain a sample of star clusters in the entire Galactic Plane with |b| < 20°. A total of 1788 star cluster candidates are identified in this survey.
D. Froebrich   +12 more
semanticscholar   +1 more source

THE CARNEGIE-IRVINE GALAXY SURVEY. III. THE THREE-COMPONENT STRUCTURE OF NEARBY ELLIPTICAL GALAXIES [PDF]

open access: yes, 2012
Motivated by recent developments in our understanding of the formation and evolution of massive galaxies, we explore the detailed photometric structure of a representative sample of 94 bright, nearby elliptical galaxies, using high-quality optical images
Song Huang   +17 more
semanticscholar   +1 more source

Space Science [PDF]

open access: yes, 2021
The all-encompassing term Space Science was coined to describe all of the various fields of research in science: Physics and astronomy, aerospace engineering and spacecraft technologies, advanced computing and radio communication systems, that are ...

core   +1 more source

THE DOUBLE PULSAR: EVIDENCE FOR NEUTRON STAR FORMATION WITHOUT AN IRON CORE-COLLAPSE SUPERNOVA [PDF]

open access: yes, 2013
The double pulsar system PSR J0737−3039A/B is a double neutron star binary, with a 2.4 hr orbital period, which has allowed measurement of relativistic orbital perturbations to high precision.
R. Ferdman   +35 more
semanticscholar   +1 more source

Earth and Space Science Open Archive Takes a Big Step Forward

open access: yesEOS, 2022
The ESS Open Archive is moving to a new publishing platform where it will continue to accelerate the open discovery of Earth and space science research.
Jonathan Jiang, Nick Violette
semanticscholar   +1 more source

The influence of the cluster environment on the star formation efficiency of 12 Virgo spiral galaxies [PDF]

open access: yes, 2012
The influence of the environment on gas surface density and star formation efficiency of cluster spiral galaxies is investigated. We extend previous work on radial profiles by a pixel-to pixel analysis looking for asymmetries due to environmental ...
B. V. .. O. I. Wong   +17 more
semanticscholar   +1 more source

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