Unveiling the 3D structure of nova shells with MUSE: The case of RR Pic
A&A, 681 (2024) A106
Published online: 2024-01-24
Articles citing this article
The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
Cited article:
This article has been cited by the following article(s):
A persistent bow shock in a diskless magnetized accreting white dwarf
Krystian Iłkiewicz, Simone Scaringi, Domitilla de Martino, Christian Knigge, Sara E. Motta, Nanda Rea, David Buckley, Noel Castro Segura, Paul J. Groot, Anna F. McLeod, Luke T. Parker and Martina VeresvarskaNature Astronomy (2026)
https://doi.org/10.1038/s41550-025-02748-8
Unveiling the 3D geometry of nova shells with MUSE
L. Celedón, L. Schmidtobreick, C. Tappert and F. SelmanRevista Mexicana de Astrofísica y Astronomía Serie de Conferencias 60 175 (2026)
https://doi.org/10.22201/ia.14052059p.2026.60.159
MUSE observations of V1425 Aql reveal an arc-shaped nova shell
Lientur Celedón, Claus Tappert, Linda Schmidtobreick and Fernando J. SelmanAstronomy & Astrophysics 694 A238 (2025)
https://doi.org/10.1051/0004-6361/202453400
VLT VIMOS integral field spectroscopy of the nova remnant FH Ser
M. A. Guerrero, E. Santamaría, L. Takeda, J. I. González-Carbajal, S. Cazzoli, A. Ederoclite and J. A. ToaláAstronomy & Astrophysics 694 A144 (2025)
https://doi.org/10.1051/0004-6361/202452743
Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It Will Be the Brightest Classical or Recurrent Nova Ever Observed in X-Rays*
S. Starrfield, M. Bose, C. E. Woodward, C. Iliadis, W. R. Hix, A. Evans, G. Shaw, D. P. K. Banerjee, T. Liimets, K. L. Page, T. R. Geballe, I. Ilyin, I. Perron and R. M. WagnerThe Astrophysical Journal 982 (2) 89 (2025)
https://doi.org/10.3847/1538-4357/adb8ed
A Photoionization Model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii
C. E. Woodward, G. Shaw, S. Starrfield, A. Evans and K. L. PageThe Astrophysical Journal 968 (1) 31 (2024)
https://doi.org/10.3847/1538-4357/ad4097
Ancient Nova Shells of RX Pup Indicate Evolution of Mass Transfer Rate
Krystian Iłkiewicz, Joanna Mikołajewska, Michael M. Shara, Jacqueline K. Faherty and Simone ScaringiThe Astrophysical Journal Letters 972 (1) L14 (2024)
https://doi.org/10.3847/2041-8213/ad6e5a
3D physical structure and angular expansion of the remnant of the recurrent nova T Pyx
E Santamaría, J A Toalá, M A Guerrero, G Ramos-Larios and L SabinMonthly Notices of the Royal Astronomical Society 530 (4) 4531 (2024)
https://doi.org/10.1093/mnras/stae1139