Zobrazeno 1 - 10
of 145
pro vyhledávání: '"Magda Arnaboldi"'
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 271, Iss 2, p 40 (2024)
Thanks to the MUSE integral field spectrograph on board the Very Large Telescope (VLT), extragalactic distance measurements with the [O iii ] λ 5007 planetary nebula luminosity function (PNLF) are now possible out to ∼40 Mpc. Here we analyze the V
Externí odkaz:
https://doaj.org/article/5a6cc1621a6e41bfb6c918e889e46ef2
Publikováno v:
The Astrophysical Journal Letters, Vol 956, Iss 1, p L14 (2023)
An outstanding question is whether the α /Fe bimodality exists in disk galaxies other than in the Milky Way. Here we present a bimodality using our state-of-the-art galactic chemical evolution models that can explain various observations in the Andr
Externí odkaz:
https://doaj.org/article/cf36960b1a764b488b095fb4c9bc8d2d
Autor:
Magda Arnaboldi, Ortwin Gerhard
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
Nearly all intragroup (IGL) and intracluster light (ICL) comes from stars that are not bound to any single galaxy but were formed in galaxies and later unbound from them. In this review we focus on the physical properties–phase space properties, me
Externí odkaz:
https://doaj.org/article/a021944c30a042788969aa32a33eb605
Publikováno v:
Galaxies, Vol 3, Iss 4, Pp 212-219 (2015)
Planetary nebulas (PNs) offer a unique tool to investigate the outer regions of massive galaxies because their strong [OIII]λ5007Å emission line makes them detectable out to several effective radii from the galaxy’s centre. We use a deep and exte
Externí odkaz:
https://doaj.org/article/889df2b4e9264239a13f8faa75fe2903
Autor:
Stefan Meingast, João Alves, Hervé Bouy, Monika G. Petr-Gotzens, Verena Fürnkranz, Josefa E. Großschedl, David Hernandez, Alena Rottensteiner, Magda Arnaboldi, Joana Ascenso, Amelia Bayo, Erik Brändli, Anthony G.A. Brown, Jan Forbrich, Alyssa Goodman, Alvaro Hacar, Birgit Hasenberger, Rainer Köhler, Karolina Kubiak, Michael Kuhn, Charles Lada, Kieran Leschinski, Marco Lombardi, Diego Mardones, Laura Mascetti, Núria Miret-Roig, André Moitinho, Koraljka Mužić, Martin Piecka, Laura Posch, Timo Prusti, Karla Peña Ramírez, Ronny Ramlau, Sebastian Ratzenböck, Germano Sacco, Cameren Swiggum, Paula Stella Teixeira, Vanessa Urban, Eleonora Zari, Catherine Zucker
VISIONS is an ESO public survey of five nearby (d < 500 pc) star-forming molecular cloud complexes that are canonically associated with the constellations of Chamaeleon, Corona Australis, Lupus, Ophiuchus, and Orion. The survey was carried out with V
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::85eaa74e6340e260150a66ed5e5fd4db
Autor:
Tayyaba Zafar, Jon Lawrence, Jessica Zheng, David Adams, Vitor N. Hartmann, Celestina Lacombe, Michael Goodwin, Nuria Lorente, Ellie O'Brien, Will Saunders, Helen McGregor, Lew Waller, Nirmala Kunwar, Daniel M. Faes, Jennifer Marshall, Darren L. DePoy, Alexandar Ji, Dennis Zaritsky, Casey Papovich, Steven Finkelstein, Andrew Szentgyorgyi, Roderik Overzier, Kyler Kuehn, Luca Cortese, Scott Croom, Sarah Martell, Matthew Colless, Anilkumar Mailvaganam, Andrew M. Hopkins, Magda Arnaboldi, Celine Peroux, Christian Johnson
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy IX.
Autor:
Alberto Micol, Magda Arnaboldi, Daniel Brandt, Nausicaa Delmotte, Vincenzo Forchì, Nathalie Fourniol, Ahmed Mubashir Kahn, Laura Mascetti, Stanislaw Podgorski, Jörg Retzlaff, Martino Romaniello, Malgorzata Stellert, Stefano Zampieri, Olivier R. Hainaut, Mauro Barbieri
Publikováno v:
Observatory Operations: Strategies, Processes, and Systems IX.
Autor:
Michael R. Merrifield, Anastasia A. Ponomareva, Magda Arnaboldi, Konrad Kuijken, Kenneth C. Freeman, Suryashree Aniyan, Ortwin Gerhard, Lodovico Coccato
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 500(3), 3579-3593. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 500(3), 3579-3593
Monthly Notices of the Royal Astronomical Society, 500(3), 3579-3593
The mass-to-light ratio (M/L) is a key parameter in decomposing galactic rotation curves into contributions from the baryonic components and the dark halo of a galaxy. One direct observational method to determine the disc M/L is by calculating the su
Autor:
Souradeep Bhattacharya, Magda Arnaboldi, Nelson Caldwell, Ortwin Gerhard, Chiaki Kobayashi, Johanna Hartke, Kenneth C Freeman, Alan W McConnachie, Puragra Guhathakurta
We obtain a magnitude-limited sample of Andromeda (M 31) disc PNe with chemical abundance estimated through the direct detection of the [OIII] 4363 $\mathring{\mathrm A}$ line. This leads to $205$ and $200$ PNe with oxygen and argon abundances respec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::732a16c9fbb6dac1db1d4570b2874883
http://arxiv.org/abs/2203.06428
http://arxiv.org/abs/2203.06428
Autor:
Antonio La Marca, Reynier Peletier, Enrichetta Iodice, Maurizio Paolillo, Nelvy Choque Challapa, Aku Venhola, Duncan A. Forbes, Michele Cantiello, Michael Hilker, Marina Rejkuba, Magda Arnaboldi, Marilena Spavone, Giuseppe D’Ago, Maria Angela Raj, Rossella Ragusa, Marco Mirabile, Roberto Rampazzo, Chiara Spiniello, Steffen Mieske, Pietro Schipani
Publikováno v:
Astronomy and astrophysics, 659:A92. EDP Sciences
At ~50 Mpc, the Hydra I cluster of galaxies is among the closest cluster in the z=0 Universe, and an ideal environment to study dwarf galaxy properties in a cluster environment. We exploit deep imaging data of the Hydra I cluster to construct a new p