Results 241 to 250 of about 77,155 (253)
New Survey of the Variable Stars in the Small Magellanic Cloud
, 1962 Cecilia Payne Gaposchkin
openalex +2 more sources
MAGELLANIC CLOUDS, X. AN EVALUATION OF THE ZERO POINT CORRECTION. [PDF]
Proc Natl Acad Sci U S A, 1954 Shapley H, Nail VM.
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Scientific American, 1985
In recent years astronomers have found a number of surprises in the structure of the Magellanic clouds themselves. Tides raised by their interaction with each other and with the Milky Way have distorted their form, and there is now a long tendril of gas and stars extending between the LMC and the SMC.
openaire +2 more sources
In recent years astronomers have found a number of surprises in the structure of the Magellanic clouds themselves. Tides raised by their interaction with each other and with the Milky Way have distorted their form, and there is now a long tendril of gas and stars extending between the LMC and the SMC.
openaire +2 more sources
1924
With the recent determination at the Harvard Observatory of standardized sequences of apparent magnitudes in the Small Magellanic Cloud, we have reached a new phase in the study of stellar organization. Having found, as one product of the photometric work, the distance of this star cloud, we are now in a position to determine for several types of stars
openaire +2 more sources
With the recent determination at the Harvard Observatory of standardized sequences of apparent magnitudes in the Small Magellanic Cloud, we have reached a new phase in the study of stellar organization. Having found, as one product of the photometric work, the distance of this star cloud, we are now in a position to determine for several types of stars
openaire +2 more sources
The Motions of the Magellanic Clouds
Publications of the Astronomical Society of the Pacific, 1944In 1917 I called attention1 to an apparent systematic difference between the radial velocities of the gaseous nebulae in the northern and southern parts of the Large Magellanic Cloud, suggesting that this difference might result from a rotation of the cloud. In 1920 Hertzsprung proposed2 the simpler explanation, namely, "that all parts of the cloud are
openaire +2 more sources
The Magellanic Clouds: Structure and Evolution of the Magellanic Clouds. [PDF]
Science, 1984 openaire +3 more sources
AGB stars in the Magellanic Clouds
Astrophysics and Space Science, 1994The stars that will be detectable in the Magellanic Clouds by the DENIS and 2MASS near infrared surveys are enumerated. All thermally-pulsing AGB stars will be observable in I, J, H and K, along with the top two magnitudes of both the early-AGB and the first giant branch.
openaire +2 more sources
Nature, 1967
The Magellanic Clouds, visible in the Southern Hemisphere, are the nearest external galaxies. Their brightest stars can be distinguished unambiguously with the spectroscope. A spectral survey of the 194 brightest known stars in the Large Magellanic Cloud has provided new information on the evolution of massive stars. Such short-lived supergiants should
openaire +2 more sources
The Magellanic Clouds, visible in the Southern Hemisphere, are the nearest external galaxies. Their brightest stars can be distinguished unambiguously with the spectroscope. A spectral survey of the 194 brightest known stars in the Large Magellanic Cloud has provided new information on the evolution of massive stars. Such short-lived supergiants should
openaire +2 more sources
Bypassing the Magellanic Cloud
Science, 1999ASTRONOMYAs the tug-of-war continues over the distance to a nearby galaxy called the Large Magellanic Cloud--a first step in the cosmic distance ladder ([see main text][1])--a few astronomers have boldly tried to leapfrog it. They are using clever geometric techniques to get absolute distances to more remote galaxies.
openaire +2 more sources
Clusters in the Magellanic Clouds
1971Star clusters are extremely common in the Magellanic Clouds. About 120 are known in the SMC, and more than 1600 in the LMC. The true number there has been estimated by Hodge and Sexton (1966) to be about 6000, this total referring to clusters with brightest stars brighter than M B=2.
openaire +2 more sources