Zobrazeno 1 - 10
of 143
pro vyhledávání: '"F Dell'Agli"'
Autor:
M. La Cognata, S. Palmerini, P. Adsley, F. Hammache, A. Di Pietro, P. Figuera, R. Alba, S. Cherubini, F. Dell'Agli, G.L. Guardo, M. Gulino, L. Lamia, D. Lattuada, C. Maiolino, A. Oliva, R.G. Pizzone, P.M. Prajapati, S. Romano, D. Santonocito, R. Spartá, M.L. Sergi, A. Tumino
Publikováno v:
Physics Letters B, Vol 826, Iss , Pp 136917- (2022)
The 26Al abundance holds a special role in present-day astrophysics, since it is a probe of active nucleosynthesis in the Galaxy and a valuable constraint of Galactic core-collapse supernovae rate. It is estimated through the detection of the 1809-ke
Externí odkaz:
https://doaj.org/article/f1f3b29797ee4b8fb716c4a2851bd416
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 519:2169-2185
We study a sample of single Galactic post-asymptotic giant branch (post-AGB) stars with known surface chemical composition. Gaia EDR3 and Gaia DR3 parallaxes have enabled accurate determinations of the luminosities of these objects, thus making it po
Autor:
A. P. Milone, G. Cordoni, A. F. Marino, F. D’Antona, A. Bellini, M. Di Criscienzo, E. Dondoglio, E. P. Lagioia, N. Langer, M. V. Legnardi, M. Libralato, H. Baumgardt, M. Bettinelli, Y. Cavecchi, R. de Grijs, L. Deng, B. Hastings, C. Li, A. Mohandasan, A. Renzini, E. Vesperini, C. Wang, T. Ziliotto, M. Carlos, G. Costa, F. Dell’Agli, S. Di Stefano, S. Jang, M. Martorano, M. Simioni, M. Tailo, P. Ventura
In the past years, we have undertaken an extensive investigation of LMC and SMC star clusters based on HST data. We present photometry and astrometry of stars in 101 fields observed with the WFC/ACS, UVIS/WFC3 and NIR/WFC3 cameras. These fields compr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f6aa121708de69bc40393058e30099e
https://hdl.handle.net/2117/386942
https://hdl.handle.net/2117/386942
Autor:
F D’Antona, F Dell’Agli, M Tailo, A P Milone, P Ventura, E Vesperini, G Cordoni, A Dotter, A F Marino
The Color Magnitude Diagram (CMD) morphology of the "extended" main sequence turnoff (eMSTO) and upper main sequence (MS) of the intermediate age ($\lesssim 2$ Gyr) Large Magellanic Cloud Cluster NGC 1783 shows the presence of a small group of UV-dim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::59542fa2deebd61c82a589642b1fd48e
http://arxiv.org/abs/2303.16049
http://arxiv.org/abs/2303.16049
Akademický článek
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Akademický článek
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Publikováno v:
Astronomy & Astrophysics. 671:A86
Context. The study of post-asymptotic giant branch (post-AGB) stars is a valuable tool in improving our understanding of poorly known aspects of the evolution of the stars throughout the asymptotic giant branch (AGB). This can be done thanks to the a
Autor:
D. A. García-Hernández, Martin Groenewegen, Lars Mattsson, F. D'Antona, Devika Kamath, M. Tailo, E. Marini, Paolo Ventura, F. Dell'Agli
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 502:L35-L39
Modelling dust formation in single stars evolving through the carbon-star stage of the asymptotic giant branch (AGB) reproduces well the mid-infrared colours and magnitudes of most of the C-rich sources in the Large Magellanic Cloud (LMC), apart from
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
Autor:
M. La Cognata, S. Palmerini, P. Adsley, F. Hammache, A. Di Pietro, P. Figuera, F. Dell’Agli, R. Alba, S. Cherubini, G. L. Guardo, M. Gulino, L. Lamia, D. Lattuada, C. Maiolino, A. Oliva, R. G. Pizzone, P. M. Prajapati, G. G. Rapisarda, S. Romano, D. Santonocito, R. Spartá, M. L. Sergi, A. Tumino, P. Ventura
The abundance of 26Al carries a special role in astrophysics, since it probes active nucleosynthesis in the Milky Way and constrains the Galactic core-collapse supernovae rate. It is estimated through the detection of the 1809 keV γ-line and from th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32a9e1a0d676115efadd04bce719c7a9
https://hdl.handle.net/11391/1544494
https://hdl.handle.net/11391/1544494