Results 91 to 100 of about 29,943 (214)

Identifying H i Emission and UV Absorber Associations near the Magellanic Stream

open access: yesThe Astrophysical Journal
We present a new technique to identify associations of H i emission in the Magellanic Stream (MS) and ultraviolet (UV) absorbers from 92 QSO sight lines near the MS. We quantify the level of associations of individual H i elements to the main H i body of
Doyeon A. Kim   +2 more
doaj   +1 more source

A Preinfall Magellanic Analog–Corona and Stream Formation in the HESTIA Cosmological Simulations

open access: yesThe Astrophysical Journal
We identify and investigate a preinfall analog of the Large and Small Magellanic Clouds (LMCs, SMCs) in the High-Resolution Environmental Simulations of the Immediate Area suite of constrained cosmological simulations.
Robin Chisholm   +5 more
doaj   +1 more source

THE ABUNDANCES OF HEAVY ELEMENTS IN RED SUPERGIANTS OF MAGELLANIC CLOUDS

open access: yesOdessa Astronomical Publications, 2013
The spectra of Magellanic Clouds (MC) supergiants PMMR23, PMMR144 and RM 1-667 with resolving power R=30,000 and signal to noise ratio near 100 obtained at3.6 metertelescope in Chile were analysed. We present are port on the  detailed investigation of MC
V. Gopka   +7 more
doaj   +1 more source

Merrill-Sanford bands in Large Magellanic Cloud carbon stars [PDF]

open access: bronze, 2004
D. H. Morgan   +2 more
openalex   +1 more source

The SDSS-V Local Volume Mapper (LVM): Scientific Motivation and Project Overview

open access: yesThe Astronomical Journal
We present the Sloan Digital Sky Survey V Local Volume Mapper (LVM). The LVM is an integral-field spectroscopic survey of the Milky Way, Magellanic Clouds, and a sample of local volume galaxies, connecting resolved parsec-scale individual sources of ...
Niv Drory   +50 more
doaj   +1 more source

Infrared excess in semi-regular variables in the Magellanic Clouds

open access: yesEPJ Web of Conferences, 2017
Following up on our recent work we are investigating if Type II Cepheids could be “hiding” in the sample of stars classified by the OGLE team as long-period variables.
Groenewegen Martin A.T.   +1 more
doaj   +1 more source

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