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Javier Lillo Alcolea on Muck Rack

Javier Lillo Alcolea

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Madrid
As seen in: El Diario, Nature, Diario ABC, MDPI, Europa Press
información de tribunales para @eldiarioes Escríbeme a jlillo@eldiario.es Antes en @abc_es y @europapress bsky.app/profile/javierlillo.bsky.social
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Articles

The 17O/18O Ratio of Post-AGB Sources: Canonical and Non-Canonical Populations

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By Javier Lillo Alcolea Verified, Elisa Masa, Miguel Santander-García, Theo Khouri
| MDPI
All articles published by MDPI are made immediately available worldwide under an open access license. No special permission is required to reuse all or part of the article published by MDPI, including figures and tables. For articles published under an open access Creative Common CC BY license, any part of the article may be reused without permission provided that the original article is clearly cited. For more information, please refer to https://www.mdpi.com/openaccess.
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M 1-92: The Death of an AGB Star Told by Its Isotopic Ratios

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By Javier Lillo Alcolea Verified, Miguel Santander-García, Elisa Masa, Valentín Bujarrabal
| MDPI
All articles published by MDPI are made immediately available worldwide under an open access license. No special permission is required to reuse all or part of the article published by MDPI, including figures and tables. For articles published under an open access Creative Common CC BY license, any part of the article may be reused without permission provided that the original article is clearly cited. For more information, please refer to https://www.mdpi.com/openaccess.
Open in Who Shared Issue with article?

The messy death of a multiple star system and the resulting planetary nebula as observed by JWST - Nature Astronomy

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By Orsola De Marco, Javier Lillo Alcolea Verified, Eric G. Blackman, Jesse Bublitz, Jan Cami, D. A. García-Hernández, Martin Guerrero, David Jones, Sun Kwok, Arturo Manchado, Mikako Matsuura, Quentin A Parker, Els A. Peeters, Matt Redman, Ashley J. Ruiter, Carmen Contreras Verified, Angela Speck, Hans Van Winckel, Eva Villaver, Jeremy Walsh, Muhammad Akashi, Stavros Akras, Isabel Aleman, Philippe Amram, Elvire De Beck, Panos Boumis, Nicholas Chornay, You-Hua Chu, Jorge García-Rojas, Joel H. Kastner, Foteini Lykou, Brent Miszalski, Shazrene S. Mohamed, Ana Monreal-Ibero, Hektor Monteiro, Christophe Morisset, Jason Nordhaus, Zara Osborn, Masaaki Otsuka, Bruno C. Quint, Guillermo Quintana-Lacaci, Laurence Sabin, Miguel Santander-García, Ivo Seitenzahl, Noam Soker, Letizia Stanghellini, Wolfgang Steffen, Jesús A. Toalá, Toshiya Ueta, Wouter Vlemmings, Roger Wesson
| Nature Verified
Abstract Planetary nebulae—the ejected envelopes of red giant stars—provide us with a history of the last, mass-losing phases of 90% of stars initially more massive than the Sun. Here we analyse images of the planetary nebula NGC 3132 from the James Webb Space Telescope (JWST) Early Release Observations. A structured, extended hydrogen halo surrounding an ionized central bubble is imprinted with spiral structures, probably shaped by a low-mass companion orbiting the central star at about 40–60 au.
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