Results 151 to 160 of about 95,570 (274)
The Dark Energy Camera Magellanic Clouds Emission-line Survey
We have used the Dark Energy Camera (DECam) on the CTIO Blanco 4 m telescope to perform a new emission-line survey of the Large Magellanic Cloud (LMC) using narrowband H α and [S ii ] filters in addition to a continuum band to create pure emission-line ...
Sean D. Points +9 more
doaj +1 more source
The Tip of the Red Giant Branch and Distance of the Magellanic Clouds: results from the DENIS survey [PDF]
We present a precise determination of the apparent magnitude of the tip of the red giant branch (TRGB) in the I (0.8 micron), J (1.25 micron), and K_S (2.15 micron) bands from the luminosity function of a sample of data extracted from the DENIS catalogue
Cioni, Maria-Rosa. L. +3 more
core +2 more sources
Proper Motions Of 47 TUC And NGC 362 Relative To The Small Magellanic Cloud [PDF]
H. J. Tucholke
openalex +1 more source
Wolf-Rayet stars in the Magellanic Clouds. V - Binaries in the Small Magellanic Cloud
Repeated spectroscopic observations of all eight W-R stars in the SMC are reported. Two of the stars are of the late, cool WN subclass, with one possibly an extreme Of star. One is definitely, the other probably, constant in radial velocity. Five early, hot WN (WNE) stars all exhibit O-type spectral lines.
openaire +1 more source
We present identifications and kinematic analysis of 7426 massive (≥8 M _⊙ ) stars in the Small Magellanic Cloud (SMC), using Gaia DR3 data. We used the Gaia ( G _BP − G _RP , G ) color–magnitude diagram to select the population of massive stars, and ...
Satoya Nakano +2 more
doaj +1 more source
The proximity of the Magellanic Clouds provides the opportunity to study interacting dwarf galaxies near a massive host, and spatial trends in their stellar population properties in particular, with a unique level of detail.
Roger E. Cohen +13 more
doaj +1 more source
The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. IX. RR Lyrae Stars in the Small Magellanic Cloud [PDF]
I. Soszyński +7 more
openalex +1 more source
Stellar winds in the Small Magellanic Cloud
According to the predictions of line-driven stellar wind theory, the mass loss from luminous stars should be proportional to some power of the metallicity, yet previous studies have not shown this effect clearly. The authors have observed 22 main-sequence and giant O-type stars n the SMC with the low-resolution mode of the IUE in order to study the ...
Catharine D. Garmany +1 more
openaire +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
An ATCA radio-continuum study of the Small Magellanic Cloud -- III. Supernova remnants and their environments [PDF]
M. D. Filipović +6 more
openalex +1 more source

