Year: 2013
Type: article
Abstract: Aims. Three-dimensional (3D) maps of the Galactic interstellar matter (ISM) are a potential tool of wide use, but accurate and detailed maps are still lacking. One of the ways to construct the maps is to invert individual distance-limited ISM measurements, a method we have applied here to measurements of stellar color excess in the optical.
Source: Astronomy and Astrophysics
Institutions: Centre National de la Recherche Scientifique, Observatoire de Paris, Galaxies, Etoiles, Physique et Instrumentation, Université Paris Diderot, ACRI Group (France), Institut des Sciences de la Terre, Institut de Recherche pour le Développement, University of Geneva, Australian National University, Mount Stromlo Observatory
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W2010333921
