Zobrazeno 1 - 10
of 286
pro vyhledávání: '"R Wesson"'
Autor:
P. Bouchet, R. Gastaud, A. Coulais, M. J. Barlow, C. Fransson, P. J. Kavanagh, J. Larsson, T. Temim, O. C. Jones, A. S. Hirschauer, T. Tikkanen, J. A. D. L. Blommaert, O. D. Fox, A. Glasse, N. Habel, J. Hjorth, J. Jaspers, O. Krause, R. M. Lau, L. Lenkić, M. Meixner, O. Nayak, A. Rest, B. Sargent, R. Wesson, G. S. Wright, L. Colina, E. F. van Dishoeck, M. Güdel, Th. Henning, P.-O. Lagage, G. Östlin, T. P. Ray, B. Vandenbussche
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 1, p 51 (2024)
There exist very few mid-infrared (IR) observations of supernovae (SNe) in general. Therefore, SN 1987A, the closest visible SN in 400 yr, gives us the opportunity to explore the mid-IR properties of SNe, the dust in their ejecta, and the surrounding
Externí odkaz:
https://doaj.org/article/523ede7d35f64fc8a49e9fd61097e41d
Autor:
J. Larsson, C. Fransson, B. Sargent, O. C. Jones, M. J. Barlow, P. Bouchet, M. Meixner, J. A. D. L. Blommaert, A. Coulais, O. D. Fox, R. Gastaud, A. Glasse, N. Habel, A. S. Hirschauer, J. Hjorth, J. Jaspers, P. J. Kavanagh, O. Krause, R. M. Lau, L. Lenkić, O. Nayak, A. Rest, T. Temim, T. Tikkanen, R. Wesson, G. S. Wright
Publikováno v:
The Astrophysical Journal Letters, Vol 949, Iss 2, p L27 (2023)
We present initial results from JWST NIRSpec integral field unit observations of the nearby supernova SN 1987A. The observations provide the first spatially resolved spectroscopy of the ejecta and equatorial ring (ER) over the 1–5 μ m range. We co
Externí odkaz:
https://doaj.org/article/4c718bd7bd004042b3c8166ca3ee0cce
Autor:
O. C. Jones, P. J. Kavanagh, M. J. Barlow, T. Temim, C. Fransson, J. Larsson, J. A. D. L. Blommaert, M. Meixner, R. M. Lau, B. Sargent, P. Bouchet, J. Hjorth, G. S. Wright, A. Coulais, O. D. Fox, R. Gastaud, A. Glasse, N. Habel, A. S. Hirschauer, J. Jaspers, O. Krause, L. Lenkić, O. Nayak, A. Rest, T. Tikkanen, R. Wesson, L. Colina, E. F. van Dishoeck, M. Güdel, Th. Henning, P.-O. Lagage, G. Östlin, T. P. Ray, B. Vandenbussche
Publikováno v:
The Astrophysical Journal, Vol 958, Iss 1, p 95 (2023)
Supernova (SN) 1987A is the nearest supernova in ∼400 yr. Using the JWST MIRI Medium Resolution Spectrograph, we spatially resolved the ejecta, equatorial ring (ER), and outer rings in the mid-infrared 12,927 days (35.4 yr) after the explosion. The
Externí odkaz:
https://doaj.org/article/32ad682312054cacb5d6830b91740247
Autor:
Maria Niculescu-Duvaz, M J Barlow, William Dunn, Antonia Bevan, Omar Ahmed, David Arkless, Jon Barker, Sidney Bartolotta, Liam Brockway, Daniel Browne, Ubaid Esmail, Max Garner, Wiktoria Guz, Scarlett King, Hayri Kose, Madeline Lampstaes-Capes, Joseph Magen, Nicole Morrison, Kyaw Oo, Balvinder Paik, Joanne Primrose, Danny Quick, Anais Radeka, Anthony Rodney, Eleanor Sandeman, Fawad Sheikh, Camron Stansfield, Delayne Symister, Joshua Taylor, William Wilshere, R Wesson, I De Looze, G C Clayton, K Krafton, M Matsuura
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 519:2940-2950
Core-collapse supernovae (CCSNe) are potentially capable of producing large quantities of dust, with strong evidence that ejecta dust masses can grow significantly over extended periods of time. Red-blue asymmetries in the broad emission lines of CCS
Akademický článek
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Akademický článek
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Autor:
J García-Rojas, C Morisset, D Jones, R Wesson, H M J Boffin, H Monteiro, R L M Corradi, P Rodríguez-Gil
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 510:5444-5463
We present MUSE deep integral-field unit spectroscopy of three planetary nebulae(PNe) with high abundance discrepancy factors (ADF > 20): NGC 6778, M 1-42 and Hf 2-2. We have constructed flux maps for more than 40 emission lines, and use them to buil
Autor:
Maria Niculescu-Duvaz, M J Barlow, A Bevan, R Wesson, D Milisavljevic, I De Looze, G C Clayton, K Krafton, M Matsuura, R Brady
Publikováno v:
Monthly Notices of the Royal Astronomical Society
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Modelling the red-blue asymmetries seen in the broad emission lines of core-collapse supernovae (CCSNe) is a powerful technique to quantify total dust mass formed in the ejecta at late times ($>5$ years after outburst) when ejecta dust temperatures b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec7930019b461ece6e31f667b17acb94
https://orca.cardiff.ac.uk/id/eprint/152108/1/stac1626.pdf
https://orca.cardiff.ac.uk/id/eprint/152108/1/stac1626.pdf
Akademický článek
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Autor:
P Scicluna, F Kemper, I McDonald, S Srinivasan, A Trejo, S H J Wallström, J G A Wouterloot, J Cami, J Greaves, Jinhua He, D T Hoai, Hyosun Kim, O C Jones, H Shinnaga, C J R Clark, T Dharmawardena, W Holland, H Imai, J Th van Loon, K M Menten, R Wesson, H Chawner, S Feng, S Goldman, F C Liu, H MacIsaac, J Tang, S Zeegers, K Amada, V Antoniou, A Bemis, M L Boyer, S Chapman, X Chen, S-H Cho, L Cui, F Dell’Agli, P Friberg, S Fukaya, H Gomez, Y Gong, M Hadjara, C Haswell, N Hirano, S Hony, H Izumiura, M Jeste, X Jiang, T Kaminski, N Keaveney, J Kim, K E Kraemer, Y-J Kuan, E Lagadec, C F Lee, D Li, S-Y Liu, T Liu, I de Looze, F Lykou, C Maraston, J P Marshall, M Matsuura, C Min, M Otsuka, M Oyadomari, H Parsons, N A Patel, E Peeters, T A Pham, J Qiu, S Randall, G Rau, M P Redman, A M S Richards, S Serjeant, C Shi, G C Sloan, M W L Smith, K-W Suh, J A Toalá, S Uttenthaler, P Ventura, B Wang, I Yamamura, T Yang, Y Yun, F Zhang, Y Zhang, G Zhao, M Zhu, A A Zijlstra
Publikováno v:
Scicluna, P, Kemper, F, Mcdonald, I, Srinivasan, S, Trejo, A, Wallström, S H J, Wouterloot, J G A, Cami, J, Greaves, J, He, J, Hoai, D T, Kim, H, Jones, O C, Shinnaga, H, Clark, C J R, Dharmawardena, T, Holland, W, Imai, H, Van loon, J T, Menten, K M, Wesson, R, Chawner, H, Feng, S, Goldman, S, Liu, F C, Macisaac, H, Tang, J, Zeegers, S, Amada, K, Antoniou, V, Bemis, A, Boyer, M L, Chapman, S, Chen, X, Cho, S, Cui, L, Dell’agli, F, Friberg, P, Fukaya, S, Gomez, H, Gong, Y, Hadjara, M, Haswell, C, Hirano, N, Hony, S, Izumiura, H, Jeste, M, Jiang, X, Kaminski, T, Keaveney, N, Kim, J, Kraemer, K E, Kuan, Y, Lagadec, E, Lee, C F, Li, D, Liu, S, Liu, T, De looze, I, Lykou, F, Maraston, C, Marshall, J P, Matsuura, M, Min, C, Otsuka, M, Oyadomari, M, Parsons, H, Patel, N A, Peeters, E, Pham, T A, Qiu, J, Randall, S, Rau, G, Redman, M P, Richards, A M S, Serjeant, S, Shi, C, Sloan, G C, Smith, M W L, Suh, K, Toalá, J A, Uttenthaler, S, Ventura, P, Wang, B, Yamamura, I, Yang, T, Yun, Y, Zhang, F, Zhang, Y, Zhao, G, Zhu, M & Zijlstra, A A 2022, ' The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope ', Monthly Notices of the Royal Astronomical Society, vol. 512, no. 1, pp. 1091-1110 . https://doi.org/10.1093/mnras/stab2860
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of $\sim$850 Galactic evolved stars within 3\,kpc at (sub-)mm wavelengths, observed in the CO $J = $ (2$-$1) and (3$-$2) rotational lines, and the sub-mm continuum, using the James Cl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e04db7415ef18a187d97aa45c66f5a8a
https://lirias.kuleuven.be/handle/20.500.12942/694375
https://lirias.kuleuven.be/handle/20.500.12942/694375