Zobrazeno 1 - 10
of 322
pro vyhledávání: '"Friedrich Wyrowski"'
Autor:
Pamela Klaassen, Maria Beltrán, Alessio Traficante, Mark Booth, Kate Pattle, Jonathan Marshall, Joshua Lovell, Brandt Gaches, Alvaro Hacar, Nicolas Peretto, Caroline Bot, Doris Arzoumanian, Thomas Stanke, Gaspard Duchêne, Ana Duarte Cabral, Antonio Hales, David Eden, Patricia Luppe, Jens Kauffmann, Elena Redaelli, Sebastian Marino, Álvaro Sánchez-Monge, Andrew Rigby, Dmitry Semenov, Eugenio Schisano, Mark Thompson, Silvia Spezzano, Claudia Cicone, Friedrich Wyrowski, Martin Cordiner, Tony Mroczkowski, Doug Johnstone, Luca Di Mascolo, Minju Lee, Eelco van Kampen, Thomas Maccarone, Daizhong Liu, Matthew Smith, Amélie Saintonge, Sven Wedemeyer, Alexander Thelen
Publikováno v:
Open Research Europe, Vol 4 (2024)
As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop a greater understanding for the complex relationships between the large-scale diffuse gas and dust in Giant Molecular Clouds (GMCs), how it moves, how it is af
Externí odkaz:
https://doaj.org/article/983f2c37d37c4607914d3fadf95c2ee1
Autor:
Roberto Galván-Madrid, Daniel J. Díaz-González, Frédérique Motte, Adam Ginsburg, Nichol Cunningham, Karl M. Menten, Mélanie Armante, Mélisse Bonfand, Jonathan Braine, Timea Csengeri, Pierre Dell’Ova, Fabien Louvet, Thomas Nony, Rudy Rivera-Soto, Patricio Sanhueza, Amelia M. Stutz, Friedrich Wyrowski, Rodrigo H. Álvarez-Gutiérrez, Tapas Baug, Sylvain Bontemps, Leonardo Bronfman, Manuel Fernández-López, Antoine Gusdorf, Atanu Koley, Hong-Li Liu, Javiera Salinas, Allison P. M. Towner, Anthony P. Whitworth
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 274, Iss 1, p 15 (2024)
We use the H41 α recombination line to create templates of the millimeter free–free emission in the ALMA-IMF continuum maps, which allows us to separate it from dust emission. This method complements spectral-index information and extrapolation fr
Externí odkaz:
https://doaj.org/article/0b10ed6f258143538914748f231323c6
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 2, p 151 (2024)
Hub–filament systems (HFSs) being the potential sites of formation of star clusters and high-mass stars, provide a testbed for the current theories that attempt to explain star formation globally. It is thus important to study a large number of HFS
Externí odkaz:
https://doaj.org/article/a72a59ed39cd4b6184c322c74c4f036f
Autor:
Jagadheep D. Pandian, Rwitika Chatterjee, Timea Csengeri, Jonathan P. Williams, Friedrich Wyrowski, Karl M. Menten
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 1, p 54 (2024)
The mass assembly in star-forming regions arises from the hierarchical structure in molecular clouds in tandem with fragmentation at different scales. In this paper, we present a study of the fragmentation of massive clumps covering a range of evolut
Externí odkaz:
https://doaj.org/article/c75c51502b904dd085893df2600cd01c
Autor:
Luis A. Zapata, Manuel Fernández-López, Silvia Leurini, Estrella Guzmán Ccolque, I. M. Skretas, Luis F. Rodríguez, Aina Palau, Karl M. Menten, Friedrich Wyrowski
Publikováno v:
The Astrophysical Journal Letters, Vol 956, Iss 2, p L35 (2023)
In the last years there has been a substantial increase in the number of the reported massive and luminous star-forming regions with related explosive outflows thanks to the superb sensitivity and angular resolution provided by the new radio, infrare
Externí odkaz:
https://doaj.org/article/3fd9e677514b4f5c80ec9703c69f9b5a
Autor:
Ramsey L. Karim, Marc W. Pound, Alexander G. G. M. Tielens, Maitraiyee Tiwari, Lars Bonne, Mark G. Wolfire, Nicola Schneider, Ümit Kavak, Lee G. Mundy, Robert Simon, Rolf Güsten, Jürgen Stutzki, Friedrich Wyrowski, Netty Honingh
Publikováno v:
The Astronomical Journal, Vol 166, Iss 6, p 240 (2023)
We investigate the physical structure and conditions of photodissociation regions (PDRs) and molecular gas within the Pillars of Creation in the Eagle Nebula using SOFIA FEEDBACK observations of the [C ii ] 158 μ m line. These observations are veloc
Externí odkaz:
https://doaj.org/article/b48e6fa67e13425bae93cf2615656ea4
Akademický článek
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Context: Supernovae (SNe) inject large amounts of energy and chemically enriched materials into their surrounding interstellar medium and, in some instances, into molecular clouds (MCs). The interaction of a supernova remnant (SNR) with a MC plays a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::640f01c7fd8e5494d5836adea1ff6038
http://arxiv.org/abs/2211.06100
http://arxiv.org/abs/2211.06100
Publikováno v:
Astronomy & Astrophysics. 673:A143
Context. Studying the physical and chemical processes leading to the formation of low-mass stars is crucial for understanding the origin of our Sun and the Solar System. In particular, analyzing the emission and absorption lines from molecules to der
Autor:
Alessio Traficante, Andrew Rigby, Timea Csengeri, Karl M. Menten, James Urquhart, K. R. Neralwar, Th. Henning, Friedrich Wyrowski, Álvaro Sánchez-Monge, Peter J. Barnes, Leonardo Bronfman, David Eden, S.-N. X. Medina, Henrik Beuther, M. Mattern, Alex R. Pettitt, Allen Y. Yang, L. D. Anderson, Adam Ginsburg, Frederic Schuller, M.-Y. Lee, Ana Duarte-Cabral, Sarah Ragan, M. Wienen, D. Colombo, C. König
The morphology of the Milky Way is still a matter of debate. In order to shed light on uncertainties surrounding the structure of the Galaxy, in this paper, we study the imprint of spiral arms on the distribution and properties of its molecular gas.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c04f4a6476a98e7b095cf0d48f8a75f2
https://hal-insu.archives-ouvertes.fr/insu-03439581
https://hal-insu.archives-ouvertes.fr/insu-03439581