The structure of a recent nova shell as observed by ALMA-Reference-Cited by-同舟云学术

The structure of a recent nova shell as observed by ALMA

Published:2018-06-30 Issue:1 Volume:480 Page:L54-L57
ISSN:1745-3925
Container-title:Monthly Notices of the Royal Astronomical Society: Letters
language:en
Short-container-title:

Author:

Diaz Marcos P¹^ORCID,Abraham Zulema¹,Ribeiro Valério A R M²³⁴,Beaklini Pedro P B¹,Takeda Larissa¹

Affiliation:

1. Departamento de Astronomia, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo (IAG/USP), Rua do Matão 1226, 05508-900, São Paulo, Brazil

2. CIDMA, Departamento de Física, Universidade de Aveiro, Campus Universitário de Santiago, P-3810-193 Aveiro, Portugal

3. Instituto de Telecomunicações, Campus Universitário de Santiago, P-3810-193 Aveiro, Portugal

4. Department of Astrophysics/IMAPP, Radboud University, PO Box 9010, NL-6500 GL Nijmegen, the Netherlands

Funder

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Foundation for Research Support of the State of São Paulo

Fundação para a Ciência e a Tecnologia

Center for Research & Development in Mathematics and Applications

Enabling Green E-science for the Square Kilometer Array Research Infrastructure

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnrasl/article-pdf/480/1/L54/25209292/sly121.pdf

Reference27 articles.

1. Near-infrared studies of the carbon monoxide and dust-forming Nova V5668 Sgr

2. Classical-Nova Contribution to the Milky Way’sAl26Abundance: Exit Channel of the KeyAl25(p,γ)Si26Resonance

3. The photoevaporation of interstellar clouds. II - Equilibrium cometary clouds

4. Classical Novae

5. Binary orbits as the driver of γ-ray emission and mass ejection in classical novae

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