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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

ptical and near-infrared data and modelling of nova V5668 Sg

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Author(s):
Takeda, L. [1] ; Diaz, M. [1] ; Campbell, R. D. [2] ; Lyke, J. E. [2] ; Lawrence, S. S. [3] ; Linford, J. D. [4] ; Sokolovsky, V, K.
Total Authors: 7
Affiliation:
[1] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, Rua Matao 1226, BR-05508900 Sao Paulo, SP - Brazil
[2] WM Keck Observ, 65-1120 Mamalahoa Highway, Kamuela, HI 96743 - USA
[3] Dept Phys & Astron, 151 Hofstra Univ, Hempstead, NY 11549 - USA
[4] Natl Radio Astron Observ, Socorro, NM 87801 - USA
Total Affiliations: 4
Document type: Journal article
Source: Monthly Notices of the Royal Astronomical Society; v. 511, n. 2, p. 1591-1600, FEB 8 2022.
Web of Science Citations: 0
Abstract

We present Hubble Space Telescope optical images, Keck-OSIRIS near-infrared (NIR) integral field spectroscopy data cubes and Keck-Near InfraRed Camera-2 (NIRC2) NIR images of nova V5668 Sgr from 2016 to 2019. The observations indicate enhanced emission at the polar caps and equatorial torus for low-ionization lines, and enhanced high-ionization emission lines only at the polar caps. The radial velocities are compatible with a homogeneous expansion velocity of v = 590 km s(-1) and a system inclination angle of 24 degrees. These values were used to estimate an expansion parallax distance of 1200 +/- 400 pc. The NIRC2 data indicate the presence of dust in 2016 and 2017, but no dust emission could be detected in 2019. The observational data were used for assembling 3D photoionization models of the ejecta. The model results indicate that the central source has a temperature of 1.88 x 10(5) K and a luminosity of 1.6 x 10(35) erg s(-1) in August of 2017 (2.4 yr post eruption), and that the shell has a mass of 6.3 x 10(-5) M-circle dot. The models also suggest anisotropy of the ionizing flux, possibly by the contribution from a luminous accretion disc. (AU)

FAPESP's process: 19/08341-8 - On the lithium mass ejected in novae: a current analysis
Grantee:Larissa Takeda
Support Opportunities: Scholarships in Brazil - Post-Doctoral