⌘+K

Pulse Explore Clubs Researchers Journals

Home Clubs Explore

March 23, 2012Astronomy and AstrophysicsOpen Access

Fundamental properties and atmospheric structure of the red supergiant VY Canis Majoris based on VLTI/AMBER spectro-interferometry

View Full Paper

Ask AI

Bookmark

Share

Abstract

Aims. We investigate the atmospheric structure and fundamental properties of the red supergiant VY CMa.

Discussion

No takes yet. Share an insight, caveat, or question.

Cite This Study

Wittkowski et al. (2012) studied this question.

synapsesocial.com/papers/6a833e332b7aeacfa1d9cb14 https://doi.org/10.1051/0004-6361/201219126

View Full Paper

Ask AI

Bookmark

Share

Keep reading

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1CO observations of a molecular cloud complex associated with the bright rim near VY Canis MajorisOriginal Research · 1978 · 45 citations
2Supergiant temperatures and linear radii from near-infrared interferometryOriginal Research · 2009 · 54 citations
3Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation ForegroundsOriginal Research · 1998 · 15,229 citations
4The ISO Long Wavelength Spectrometer line spectrum of VY Canis Majoris and other oxygen-rich evolved starsOriginal Research · 2009 · 16 citations
5DISTANCE AND KINEMATICS OF THE RED HYPERGIANT VY CMa: VERY LONG BASELINE ARRAY AND VERY LARGE ARRAY ASTROMETRYOriginal Research · 2011 · 87 citations