Results 161 to 170 of about 325,968 (275)
Observations of a Magellanic Corona. [PDF]
Krishnarao D+8 more
europepmc +1 more source
NGC 643: A New Outlying Cluster of the Small Magellanic Cloud [PDF]
G. de Vaucouleurs
openalex +1 more source
Mass-loss Rate of Highly Evolved Stars in the Magellanic Clouds
Asymptotic giant branch stars (AGBs) and red supergiant stars (RSGs) exhibit significant mass-loss phenomena and are considered important sources of interstellar dust.
Jing Wen+5 more
doaj +1 more source
Emission Objects in the Small Magellanic Cloud showing the N1, N2 Nebular Lines [PDF]
E. M. Lindsay
openalex +1 more source
The structure of the Small Magellanic Cloud. II
Multiobject fiber-optic spectroscopic observations are used to obtain system velocities and distances of 61 Cepheids in three 40-deg-diameter fields in the bar of the SMC. The Cepheid distance measurements indicate that the SMC has a depth of about 20 kpc and that the northeastern section of the bar is 10-15 kpc closer than the southern section ...
D. S. Mathewson+2 more
openaire +2 more sources
The granulation of red supergiants (RSGs) in the Magellanic Clouds is systematically investigated by combining the latest RSG samples and light curves from the Optical Gravitational Lensing Experiment and the All-Sky Automated Survey for Supernovae.
Zehao Zhang+4 more
doaj +1 more source
Nationwide Survey about the Occurrence of Aspergillosis in Captive Penguins in Zoos and Aquariums in Japan. [PDF]
Itoh M+6 more
europepmc +1 more source
The infall of the Large Magellanic Cloud (LMC) into the Milky Way’s halo impacts the distribution of stars and dark matter (DM) in our Galaxy. Mapping the observational consequences of this encounter can inform us about the properties of both galaxies ...
Manuel Cavieres+8 more
doaj +1 more source
"Fermi" bubbles are bursting from our galaxy. Their origins remain a mystery. [PDF]
Mann A.
europepmc +1 more source