Zobrazeno 1 - 10
of 3 286 261
pro vyhledávání: '"l, t"'
Autor:
Lewis, Briley, Li, Yiting, Gibbs, Aidan, Fitzgerald, Michael P., Brandt, Timothy, Gagliuffi, Daniella Bardalez, An, Qier, Chen, Minghan, Bowens-Rubin, Rachel, Salama, Maissa, Lozi, Julien, Jensen-Clem, Rebecca, Mazin, Ben
Brown dwarfs with measured dynamical masses and spectra from direct imaging are benchmarks that anchor substellar atmosphere cooling and evolution models. We present Subaru SCExAO/CHARIS infrared spectroscopy of HIP 93398 B, a brown dwarf companion r
Externí odkaz:
http://arxiv.org/abs/2411.06003
Publikováno v:
L&T Finance Holdings Ltd MarketLine Company Profile. 3/20/2024, p1-19. 19p.
Publikováno v:
L&T Finance Holdings Ltd MarketLine Company Profile. 11/24/2023, p1-19. 19p.
Autor:
Bickle, Thomas P., Schneider, Adam C., Gagné, Jonathan, Faherty, Jacqueline K., Rothermich, Austin, Vos, Johanna M., Suárez, Genaro, Kirkpatrick, J. Davy, Meisner, Aaron M., Kuchner, Marc J., Burgasser, Adam J., Marocco, Federico, Casewell, Sarah L., Caselden, Dan, Gagliuffi, Daniella Bardalez, Worlds, The Backyard, Collaboration, Planet 9
We present the discovery of VHS J183135.58$-$551355.9 (hereafter VHS J1831$-$5513), an L/T transition dwarf identified as a result of its unusually red near-infrared colors ($J-K_{\rm S}=3.633\pm0.277$ mag; $J-W2=6.249\pm0.245$ mag) from the VISTA He
Externí odkaz:
http://arxiv.org/abs/2405.03849
In the present work, we obtain the hydrostatic equilibrium configurations of neutron stars in the recently proposed $f(R,\mathcal{L},T)$ theory of gravity, for which $R$ is the Ricci scalar, $\mathcal{L}$ is the matter lagrangian density, $T$ is the
Externí odkaz:
http://arxiv.org/abs/2402.15395
Publikováno v:
L&T Finance Holdings Ltd MarketLine Company Profile. 11/30/2022, p1-17. 17p.
Autor:
Gratton, R., Bonavita, M., Mesa, D., Zurlo, A., Marino, S., Desidera, S., D'Orazi, V., Rigliaco, E., Squicciarini, V., Nogueira, P. H.
Dynamical masses of young planets aged between 10 and 200 Myr detected in imaging play a crucial role in shaping models of giant planet formation. Regrettably, only a few such objects possess these characteristics. Furthermore, the evolutionary patte
Externí odkaz:
http://arxiv.org/abs/2402.09067