Results 101 to 110 of about 30,812 (255)
Context. Surface brightness–colour relations (SBCRs) are widely used to estimate the angular diameters of stars. In particular, they are employed in the Baade–Wesselink distance determination method, which relies on the comparison between the linear and ...
Bailleul M. C. +14 more
doaj +1 more source
Cold neutral hydrogen (H i ) is a crucial precursor for molecular gas formation and can be studied via H i absorption. This study investigates H i absorption in low column density regions of the Small and Large Magellanic Clouds (SMC and LMC) using the ...
Hongxing Chen +20 more
doaj +1 more source
Orbits of LMC/SMC with recent ground-based proper motions
In recent years, with new ground-based and HST measurements of proper motions of the Magellanic Clouds being published, a need of a reanalysis of possible orbital history has arisen.
Růžička A. +3 more
doaj +1 more source
Hierarchical star formation in the Magellanic Clouds with the VMC survey. [PDF]
Miller AE +4 more
europepmc +1 more source
VLT/UVES Observations of Interstellar Molecules and Diffuse Bands in the Magellanic Clouds
We discuss the abundances of interstellar CH, CH+, and CN in the Magellanic Clouds (MC), derived from spectra of 7 SMC and 13 LMC stars obtained (mostly) with the VLT/UVES.
Adamson A. J. +35 more
core +1 more source
Distance scale calibration based on early-type binaries
Our main goal is to establish a firm empirical calibration of the surface brightness vs. (V-K) color relation for early type stars based on high quality spectroscopic and infrared observations of early-type detached eclipsing systems in the Large ...
Taormina Mónica +4 more
doaj +1 more source
Absolute Proper Motion of the Fornax Dwarf Spheroidal Galaxy from Photographic and HST WFPC2 Data
We have measured the absolute proper motion of the Fornax dwarf spheroidal galaxy from a combination of photographic plate material and HST WFPC2 data that provide a time baseline of up to 50 years.
Brian A. Keeney +9 more
core +2 more sources
The Small Magellanic Cloud [PDF]
In 1957 a two-year photometric study of the Small Magellanic Cloud, sponsored by Indiana University and supported by the National Science Foundation was completed. Six region swere investigated. They are three on the edge of the SMC centered on conspicuous star clusters and three nearer the center.
openaire +1 more source
Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source
We present the first systematic analysis comparing the ages, reddening, and radial velocities of star clusters using two widely used tools: STARLIGHT and Analyzer of Spectra for Age Determination (A.S.A.D). Both tools utilize the full integrated spectrum
Martina I. Tapia-Reina +3 more
doaj +1 more source

