Spatially resolved multiwavelength models of nova shells

• Grant number: 15/16489-4
• Support Opportunities: Research Grants - Visiting Researcher Grant - International
• Start date: November 02, 2015
• End date: December 01, 2015
• Field of knowledge: Physical Sciences and Mathematics - Astronomy - Stellar Astrophysics
• Principal Investigator: Marcos Perez Diaz
• Grantee: Marcos Perez Diaz
• Visiting researcher: Valerio Alipio Roberts Machado Ribeiro
• Visiting researcher institution: Radboud University Nijmegen, Netherlands
• Host Institution: Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG). Universidade de São Paulo (USP). São Paulo , SP, Brazil

Abstract

Significant advances in photoionization modelling of nova shells are currently possible due to adaptive optics observations and 3D physical simulation codes. A multi wavelength approach is being pursued in this collaboration, by merging both optical and radio observations in the modelling process. (AU)

Scientific publications

(References retrieved automatically from Web of Science and SciELO through information on FAPESP grants and their corresponding numbers as mentioned in the publications by the authors)

DIAZ, MARCOS P.; ABRAHAM, ZULEMA; RIBEIRO, VALERIO A. R. M.; BEAKLINI, PEDRO P. B.; TAKEDA, LARISSA. The structure of a recent nova shell as observed by ALMA. Monthly Notices of the Royal Astronomical Society, v. 480, n. 1, p. L54-L57, OCT 2018. (09/54006-4, 14/07460-0, 15/16489-4, 14/10326-3)