Catching a grown-up starfish planetary nebula – II. Plasma analysis and central star properties of PC 22

Autor: L Sabin, V Gómez-Llanos, C Morisset, V M A Gómez-González, M A Guerrero, H Todt, X Fang

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
instname

After performing the morpho-kinematic analysis of the planetary nebula (PN) PC 22, we now present its nebular and stellar analysis. The plasma investigation relies on the novel use of a Monte Carlo analysis associated with the PYNEB code for the unce

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::601533685023f120b0c0d1142afdc081
https://doi.org/10.1093/mnras/stab3649

Planetary nebulae with Wolf-Rayet-type central stars -- III. A detailed view of NGC 6905 and its central star

Autor: Laurence Sabin, Y. D. Mayya, V. M. A. Gómez-González, G. Rubio, Martín A. Guerrero, H. Todt, V. Gómez-Llanos, Gerardo Ramos-Larios, Jesús A. Toalá

Publikováno v: Digital.CSIC. Repositorio Institucional del CSIC
instname

We present a multiwavelength characterization of the planetary nebula (PN) NGC 6905 and its [Wolf–Rayet]-type ([WR]) central star (CSPN) HD 193949. Our Nordic Optical Telescope Alhambra Faint Object Spectrograph and Camera (ALFOSC) spectra and imag

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a0c4282ce157631a8c2d5598ca587e5c

Atomic Data Assessment with PyNeb

Autor: Manuel A. Bautista, Jorge García-Rojas, V. Gómez-Llanos, Christophe Morisset, Claudio Mendoza, Valentina Luridiana

Publikováno v: Atoms, Vol 8, Iss 66, p 66 (2020)
Atoms
Volume 8
Issue 4

PyNeb is a Python package widely used to model emission lines in gaseous nebulae. We take advantage of its object-oriented architecture, class methods, and historical atomic database to structure a practical environment for atomic data assessment. Ou

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::663ed969a5475fe8157ccbf129731ccb
http://arxiv.org/abs/2009.10586

SIGNALS: I. Survey description

Autor: Roberto Cid Fernandes, M. Girard, A. Luiz de Amorim, I. Millan, Martin Bureau, P. Amram, Eric W. Pellegrini, Gilles Joncas, Anne Pellerin, Francoise Combes, Hugo Martel, Julie Hlavacek-Larrondo, Dimitrios A. Gouliermis, B. Mazzilli-Ciraulo, Thomas Martin, Jorge Iglesias-Páramo, Christophe Morisset, Andreea Petric, S. Duarte Puertas, Marianne Takamiya, Rieko Momose, T. Ruiz Lara, Pauline Barmby, A. F. McLeod, I-Ting Ho, Fumi Egusa, Laurie Rousseau-Nepton, Ralf S. Klessen, Benoît Epinat, Mercedes Mollá, Angela Adamo, C. Robert, Isabel Pérez, Alexandre Alarie, A. K. Pati, Alessandro Boselli, Laurent Chemin, Grazyna Stasinska, L. Sánchez-Menguiano, Lijie Liu, Simon Prunet, Zacharie Sie Kam, Victor F. Ksoll, Kathryn Grasha, Clare Higgs, J. D. Lyman, Q. Liu, L. Della Bruna, Henri Plana, I. Moumen, N. Vale Asari, V. Gómez Llanos, Daniel Rahner, Hsi-An Pan, Fabio Bresolin, Anne-Laure Melchior, Laurent Drissen, José M. Vílchez, Robert C. Kennicutt, Kristine Spekkens, C. Crowder, R. P. Martin, Sophia Lianou, P. Karera

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2019, 489 (4), pp.5530-5546. ⟨10.1093/mnras/stz2455⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 489 (4), pp.5530-5546. ⟨10.1093/mnras/stz2455⟩
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Digital.CSIC. Repositorio Institucional del CSIC
Physics and Astronomy Publications

SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing programme designed to investigate massive star formation and HII regions in a sample of local extended galaxies. The programme will use the imaging F

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ea4060ea72d95230b1152eb47c10508
https://doi.org/10.1093/mnras/stz2455

Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.