Zobrazeno 1 - 10
of 4 743
pro vyhledávání: '"Sartorio A"'
Autor:
Liu, Boyuan, Hartwig, Tilman, Sartorio, Nina S., Dvorkin, Irina, Costa, Guglielmo, Santoliquido, Filippo, Fialkov, Anastasia, Klessen, Ralf S., Bromm, Volker
The gravitational wave (GW) signal from binary black hole (BBH) mergers is a promising probe of Population III (Pop III) stars. To fully unleash the power of the GW probe, one important step is to understand the relative importance and features of di
Externí odkaz:
http://arxiv.org/abs/2406.17397
Effective exploration abilities are fundamental for robot swarms, especially when small, inexpensive robots are employed (e.g., micro- or nano-robots). Random walks are often the only viable choice if robots are too constrained regarding sensors and
Externí odkaz:
http://arxiv.org/abs/2406.13641
Autor:
Rho, J., Park, S. -H., Arendt, R., Matsuura, M., Milisavljevic, D., Temim, T., De Looze, I., Blair, W. P., Rest, A., Fox, O., Ravi, A. P., Koo, B. -C., Barlow, M., Burrows, A., Chevalier, R., Clayton, G., Fesen, R., Fransson, C., Fryer, C., Gomez, H. L., Janka, H. -T., Kirchschlarger, F., Laming, J. M., Orlando, S., Patnaude, D., Pavlov, G., Plucinsky, P., Posselt, B., Priestley, F., Raymond, J., Sartorio, N., Schmidt, F., Slane, P., Smith, N., Sravan, N., Vink, J., Weil, K., Wheeler, J., Yoon, S. C.
We present JWST NIRCam (F356W and F444W filters) and MIRI (F770W) images and NIRSpec- IFU spectroscopy of the young supernova remnant Cassiopeia A (Cas A). We obtained the data as part of a JWST survey of Cas A. The NIRCam and MIRI images map the spa
Externí odkaz:
http://arxiv.org/abs/2406.03685
Autor:
Kirchschlager, Florian, Sartorio, Nina, De Looze, Ilse, Barlow, M. J., Schmidt, Franziska, Priestley, Felix
The expanding ejecta of supernova remnants (SNRs) are believed to form dust in dense clumps of gas. Before the dust can be expelled into the interstellar medium and contribute to the interstellar dust budget, it has to survive the reverse shock that
Externí odkaz:
http://arxiv.org/abs/2402.00701
Autor:
Milisavljevic, Dan, Temim, Tea, De Looze, Ilse, Dickinson, Danielle, Laming, J. Martin, Fesen, Robert, Raymond, John C., Arendt, Richard G., Vink, Jacco, Posselt, Bettina, Pavlov, George G., Fox, Ori D., Pinarski, Ethan, Subrayan, Bhagya, Schmidt, Judy, Blair, William P., Rest, Armin, Patnaude, Daniel, Koo, Bon-Chul, Rho, Jeonghee, Orlando, Salvatore, Janka, Hans-Thomas, Andrews, Moira, Barlow, Michael J., Burrows, Adam, Chevalier, Roger, Clayton, Geoffrey, Fransson, Claes, Fryer, Christopher, Gomez, Haley L., Kirchschlager, Florian, Lee, Jae-Joon, Matsuura, Mikako, Niculescu-Duvaz, Maria, Pierel, Justin D. R., Plucinsky, Paul P., Priestley, Felix D., Ravi, Aravind P., Sartorio, Nina S., Schmidt, Franziska, Shahbandeh, Melissa, Slane, Patrick, Smith, Nathan, Weil, Kathryn, Wesson, Roger, Wheeler, J. Craig
Publikováno v:
ApJL 965 (2024) L27 (21pp)
We present initial results from a JWST survey of the youngest Galactic core-collapse supernova remnant Cassiopeia A (Cas A), made up of NIRCam and MIRI imaging mosaics that map emission from the main shell, interior, and surrounding circumstellar/int
Externí odkaz:
http://arxiv.org/abs/2401.02477
Autor:
Kapoor, Anand Utsav, Baes, Maarten, van der Wel, Arjen, Gebek, Andrea, Camps, Peter, Nersesian, Angelos, Meidt, Sharon E., Smith, Aaron, Vicens, Sebastien, D'Eugenio, Francesco, Martorano, Marco, Barrientos, Daniela, Sartorio, Nina Sanches
We present and publicly release a new star-forming regions emission library TODDLERS (Time evolution of Observables including Dust Diagnostics and Line Emission from Regions containing young Stars) for the publicly available radiative transfer code S
Externí odkaz:
http://arxiv.org/abs/2310.00388
X-ray binaries (XRBs) are thought to regulate cosmic thermal and ionization histories during the Epoch of Reionization and Cosmic Dawn ($z\sim 5-30$).Theoretical predictions of the X-ray emission from XRBs are important for modelling such early cosmi
Externí odkaz:
http://arxiv.org/abs/2308.06154
Publikováno v:
Therapeutics and Clinical Risk Management, Vol 2016, Iss Issue 1, Pp 873-881 (2016)
Graziano Grugni,1,2 Alessandro Sartorio,1,2 Antonino Crinò3 1Division of Auxology, 2Experimental Laboratory for Auxo-endocrinological Research, San Giuseppe Hospital, Istituto Auxologico Italiano, Verbania, 3Autoimmune Endocrine Diseases Unit, Bambi
Externí odkaz:
https://doaj.org/article/9f9191f3b917441e9e3cdef1d54a959c
Autor:
Sartorio, Nina S., Fialkov, A., Hartwig, T., Mirouh, G. M., Izzard, R. G., Magg, M., Klessen, R. S., Glover, S. C. O., Chen, L., Tarumi, Y., Hendriks, D. D.
The first population of X-ray binaries (XRBs) is expected to affect the thermal and ionization states of the gas in the early Universe. Although these X-ray sources are predicted to have important implications for high-redshift observable signals, su
Externí odkaz:
http://arxiv.org/abs/2303.03435
Publikováno v:
MNRAS, 525, 348-363 (2023)
On large cosmological scales, anisotropic gravitational collapse is manifest in the dark cosmic web. Its statistical properties are little known for alternative dark matter models such as fuzzy dark matter (FDM). In this work, we assess for the first
Externí odkaz:
http://arxiv.org/abs/2301.09762