Work

ALMA observations of TiO2around VY Canis Majoris

Year: 2015

Type: article

Abstract: Context. Titanium dioxide, TiO2, is a refractory species that could play a crucial role in the dust-condensation sequence around oxygen-rich evolved stars. To date, gas phase TiO2 has been detected only in the complex environment of the red supergiant VY CMa.

Source: Astronomy and Astrophysics

DOI: 10.1051/0004-6361/201525990

Authors: E. De Beck, W. Vlemmings, S. Muller, J. H. Black, E. O’Gorman, A. M. S. Richards, A. Baudry, M. Maercker, L. Decin, E. M. Humphreys

Institutions: Chalmers University of Technology, University of Manchester, Centre National de la Recherche Scientifique, Université de Bordeaux, Laboratoire d'Astrophysique de Bordeaux, University of Amsterdam, KU Leuven, European Southern Observatory

Language: English

Topic: Astrophysics and Star Formation Studies

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: bronze

Funders: National Science Foundation, National Radio Astronomy Observatory, National Science Council, National Astronomical Observatory of Japan, Science and Technology Facilities Council, National Institutes of Natural Sciences, FP7 Ideas: European Research Council

Awards: Support for the UK ALMA Regional Centre Node, G4104599821, Magnetic fields and the outflows during the formation and evolution of stars

OpenAlex ID: W1641908580

FWCI: 3.185

Cites: 30

Cited by: 40

Related to: 10