Zobrazeno 1 - 10
of 86
pro vyhledávání: '"Daniel, Harsono"'
Autor:
Jennifer B. Bergner, J. A. Sturm, Elettra L. Piacentino, M. K. McClure, Karin I. Öberg, A. C. A. Boogert, E. Dartois, M. N. Drozdovskaya, H. J. Fraser, Daniel Harsono, Sergio Ioppolo, Charles J. Law, Dariusz C. Lis, Brett A. McGuire, Gary J. Melnick, Jennifer A. Noble, M. E. Palumbo, Yvonne J. Pendleton, Giulia Perotti, Danna Qasim, W. R. M. Rocha, E. F. van Dishoeck
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 2, p 166 (2024)
Planet formation is strongly influenced by the composition and distribution of volatiles within protoplanetary disks. With JWST, it is now possible to obtain direct observational constraints on disk ices, as recently demonstrated by the detection of
Externí odkaz:
https://doaj.org/article/0df08b8f52764a7b895eef7995c628ed
Autor:
Xianjin Shen, Hong-Li Liu, Zhiyuan Ren, Anandmayee Tej, Di Li, Hauyu Baobab Liu, Gary A. Fuller, Jinjin Xie, Sihan Jiao, Aiyuan Yang, Patrick M. Koch, Fengwei Xu, Patricio Sanhueza, Pham Ngoc Diep, Nicolas Peretto, R. K. Yadav, Busaba H. Kramer, Koichiro Sugiyama, Mark G. Rawlings, Chang Won Lee, Ken’ichi Tatematsu, Daniel Harsono, David Eden, Woojin Kwon, Chao-Wei Tsai, Glenn J. White, Kee-Tae Kim, Tie Liu, Ke Wang, Siju Zhang, Wenyu Jiao, Dongting Yang, Swagat R. Das, Jingwen Wu, Chen Wang
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 2, p 239 (2024)
Filaments are believed to play a key role in high-mass star formation. We present a systematic study of the filaments and their hosting clumps in the G35 molecular complex using James Clerk Maxwell Telescope SCUBA-2 850 μ m continuum data. We identi
Externí odkaz:
https://doaj.org/article/b7338c969125470e841ebcb8e71b6938
Autor:
Yangfan Shi, Feng Long, Gregory J. Herczeg, Daniel Harsono, Yao Liu, Paola Pinilla, Enrico Ragusa, Doug Johnstone, Xue-Ning Bai, Ilaria Pascucci, Carlo F. Manara, Gijs D. Mulders, Lucas A. Cieza
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 1, p 59 (2024)
High angular resolution imaging by Atacama Large Millimeter/submillimeter Array (ALMA) has revealed the near universality and diversity of substructures in protoplanetary disks. However, disks around M-type pre-main-sequence stars are still poorly sa
Externí odkaz:
https://doaj.org/article/4491a9018b4a454a95b55d095a3db783
Autor:
Daniel Harsono, Feng Long, Paola Pinilla, Alessia A. Rota, Carlo F. Manara, Gregory J. Herczeg, Doug Johnstone, Giovanni Rosotti, Giuseppe Lodato, Francois Menard, Marco Tazzari, Yangfan Shi
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 1, p 28 (2024)
While the most exciting explanation of the observed dust asymmetries in protoplanetary disks is the presence of protoplanets, other mechanisms can also form the dust features. This paper presents dual-wavelength Atacama Large Millimeter/submillimeter
Externí odkaz:
https://doaj.org/article/93e26bb357b14902a906cc7a35980b72
Autor:
Jeong-Eun Lee, Tomoaki Matsumoto, Hyun-Jeong Kim, Seokho Lee, Daniel Harsono, Jaehan Bae, Neal J. Evans II, Shu-ichiro Inutsuka, Minho Choi, Ken’ichi Tatematsu, Jae-Joon Lee, Daniel Jaffe
Publikováno v:
The Astrophysical Journal, Vol 953, Iss 1, p 82 (2023)
Most stars form in multiple-star systems. For a better understanding of their formation processes, it is important to resolve the individual protostellar components and the surrounding envelope and disk material at the earliest possible formation epo
Externí odkaz:
https://doaj.org/article/0d6a8ad6baf84827bc1d8e0647bc8906
Autor:
Feng Long, Bin B. Ren, Nicole L. Wallack, Daniel Harsono, Gregory J. Herczeg, Paola Pinilla, Dimitri Mawet, Michael C. Liu, Sean M. Andrews, Xue-Ning Bai, Sylvie Cabrit, Lucas A. Cieza, Doug Johnstone, Jarron M. Leisenring, Giuseppe Lodato, Yao Liu, Carlo F. Manara, Gijs D. Mulders, Enrico Ragusa, Steph Sallum, Yangfan Shi, Marco Tazzari, Taichi Uyama, Kevin Wagner, David J. Wilner, Jerry W. Xuan
Publikováno v:
The Astrophysical Journal, Vol 949, Iss 1, p 27 (2023)
Planet formation imprints signatures on the physical structures of disks. In this paper, we present high-resolution (∼50 mas, 8 au) Atacama Large Millimeter/submillimeter Array observations of 1.3 mm dust continuum and CO line emission toward the d
Externí odkaz:
https://doaj.org/article/884a898a5cb34867ba6028f8bcd6a59a
Autor:
John J. Tobin, Merel L. R. van ’t Hoff, Margot Leemker, Ewine F. van Dishoeck, Teresa Paneque-Carreño, Kenji Furuya, Daniel Harsono, Magnus V. Persson, L. Ilsedore Cleeves, Patrick D. Sheehan, Lucas Cieza
Publikováno v:
Nature. 615:227-230
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0d1ad080cc7e5f6d2692d2e4dc480df0
https://doi.org/10.1038/s41586-022-05676-z
https://doi.org/10.1038/s41586-022-05676-z
Autor:
Jane Huang, Christian Ginski, Myriam Benisty, Bin Ren, Alexander J. Bohn, Élodie Choquet, Karin I. Öberg, Álvaro Ribas, Jaehan Bae, Edwin A. Bergin, Til Birnstiel, Yann Boehler, Stefano Facchini, Daniel Harsono, Michiel Hogerheijde, Feng Long, Carlo F. Manara, François Ménard, Paola Pinilla, Christophe Pinte, Christian Rab, Jonathan P. Williams, Alice Zurlo
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2022, 930, ⟨10.3847/1538-4357/ac63ba⟩
The Astrophysical Journal, 930(2):171
Astrophysical Journal, 930(2):171. IOP Publishing Ltd.
The Astrophysical Journal, 2022, 930, ⟨10.3847/1538-4357/ac63ba⟩
The Astrophysical Journal, 930(2):171
Astrophysical Journal, 930(2):171. IOP Publishing Ltd.
While protoplanetary disks are often treated as isolated systems in planet formation models, observations increasingly suggest that vigorous interactions between Class II disks and their environments are not rare. DO Tau is a T Tauri star that has pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::82b4b3ae6d40a7696c1ccd5aa7632c69
https://hdl.handle.net/2434/929484
https://hdl.handle.net/2434/929484
Autor:
Merel L. R. van ’t Hoff, Daniel Harsono, Martijn L. van Gelder, Tien-Hao Hsieh, John J. Tobin, Sigurd S. Jensen, Naomi Hirano, Jes K. Jørgensen, Edwin A. Bergin, Ewine F. van Dishoeck
Publikováno v:
The Astrophysical Journal, 924(1):5
Van ’t Hoff, M L R, Harsono, D, Van Gelder, M L, Hsieh, T, Tobin, J J, Jensen, S S, Hirano, N, Jørgensen, J K, Bergin, E A & Van Dishoeck, E F 2022, ' Imaging the Water Snowline around Protostars with Water and HCO + Isotopologues ', Astrophysical Journal, vol. 924, no. 1, 5 . https://doi.org/10.3847/1538-4357/ac3080
Van ’t Hoff, M L R, Harsono, D, Van Gelder, M L, Hsieh, T, Tobin, J J, Jensen, S S, Hirano, N, Jørgensen, J K, Bergin, E A & Van Dishoeck, E F 2022, ' Imaging the Water Snowline around Protostars with Water and HCO + Isotopologues ', Astrophysical Journal, vol. 924, no. 1, 5 . https://doi.org/10.3847/1538-4357/ac3080
The water snowline location in protostellar envelopes provides crucial information about the thermal structure and the mass accretion process as it can inform about the occurrence of recent (≲1000 yr) accretion bursts. In addition, the ability to i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7f8c46cb714d9954a9f0f913b4df39bc
https://hdl.handle.net/1887/3561996
https://hdl.handle.net/1887/3561996
Autor:
Daniel Harsono, Yuan Chen, Benoît Tabone, Ewine F. van Dishoeck, Nadia M. Murillo, Łukasz Tychoniec, Charles L. H. Hull, John J. Tobin, Merel L. R. van ’t Hoff, Martijn L. van Gelder, Michiel R. Hogerheijde
Publikováno v:
Astronomy & Astrophysics, 655, 1-38. {EDP} Sciences
Astronomy & Astrophysics, 655:A65. EDP Sciences
Astronomy & Astrophysics, 655:A65. EDP Sciences
The physical and chemical conditions in Class 0/I protostars are fundamental in unlocking the protostellar accretion process and its impact on planet formation. The aim is to determine which physical components are traced by different molecules at su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88d73175ba6fecddaff7413a6d6e4ccd
https://hdl.handle.net/1887/3270867
https://hdl.handle.net/1887/3270867