The Initial Mass Function Based on the Full-sky 20-pc Census of \(\sim\)3,600 Stars and Brown Dwarfs

A complete accounting of nearby objects -- from the highest-mass white dwarf progenitors down to low-mass brown dwarfs -- is now possible, thanks to an almost complete set of trigonometric parallax determinations from Gaia, ground-based surveys, and Spitzer follow-up. We create a census of objects w...

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Veröffentlicht in:arXiv.org 2023-12
Hauptverfasser: J Davy Kirkpatrick, Marocco, Federico, Gelino, Christopher R, Yadukrishna Raghu, Faherty, Jacqueline K, Daniella C Bardalez Gagliuffi, Schurr, Steven D, Apps, Kevin, Schneider, Adam C, Meisner, Aaron M, Kuchner, Marc J, Caselden, Dan, Smart, R L, Casewell, S L, Raddi, Roberto, Kesseli, Aurora, Nikolaj Stevnbak Andersen, Antonini, Edoardo, Beaulieu, Paul, Bickle, Thomas P, Bilsing, Martin, Chieng, Raymond, Guillaume, Colin, Deen, Sam, Dereveanco, Alexandru, Doll, Katharina, Durantini Luca, Hugo A, Frazer, Anya, Gantier, Jean Marc, Gramaize, Léopold, Grant, Kristin, Hamlet, Leslie K, Higashimura, Hiro, Hyogo, Michiharu, Jałowiczor, Peter A, Jonkeren, Alexander, Kabatnik, Martin, Kiwy, Frank, Martin, David W, Michaels, Marianne N, Pendrill, William, Celso Pessanha Machado, Pumphrey, Benjamin, Rothermich, Austin, Russwurm, Rebekah, Sainio, Arttu, Sanchez, John, Sapelkin-Tambling, Fyodor Theo, Schümann, Jörg, Selg-Mann, Karl, Singh, Harshdeep, Stenner, Andres, Sun, Guoyou, Tanner, Christopher, Thévenot, Melina, Ventura, Maurizio, Voloshin, Nikita V, Walla, Jim, Wedracki, Zbigniew, Adorno, Jose I, Aganze, Christian, Allers, Katelyn N, Brooks, Hunter, Burgasser, Adam J, Calamari, Emily, Connor, Thomas, Costa, Edgardo, Eisenhardt, Peter R, Gagné, Jonathan, Gerasimov, Roman, Gonzales, Eileen C, Hsu, Chih-Chun, Kiman, Rocio, Li, Guodong, Low, Ryan, Mamajek, Eric, Pantoja, Blake M, Popinchalk, Mark, Rees, Jon M, Stern, Daniel, Suárez, Genaro, Theissen, Christopher, Chao-Wei, Tsai, Vos, Johanna M, Zurek, David, The Backyard Worlds, Planet 9 Collaboration
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Zusammenfassung:A complete accounting of nearby objects -- from the highest-mass white dwarf progenitors down to low-mass brown dwarfs -- is now possible, thanks to an almost complete set of trigonometric parallax determinations from Gaia, ground-based surveys, and Spitzer follow-up. We create a census of objects within a Sun-centered sphere of 20-pc radius and check published literature to decompose each binary or higher-order system into its separate components. The result is a volume-limited census of \(\sim\)3,600 individual star formation products useful in measuring the initial mass function across the stellar (\(
ISSN:2331-8422