Zobrazeno 1 - 10
of 796
pro vyhledávání: '"Mckee, Christopher"'
We analyze measurements of the thermal Sunyaev-Zeldovich (tSZ) effect arising in the circumgalactic medium (CGM) of $L^*$ galaxies, reported by Bregman et al. 2022 and Das et al. 2023. In our analysis we use the Faerman et al. 2017 and Faerman et al.
Externí odkaz:
http://arxiv.org/abs/2403.09476
Nitrogen-enriched, highly-pressurized nebular clouds surrounding a super star cluster at cosmic noon
Publikováno v:
ApJ 957 77 (2023)
Strong lensing offers a precious opportunity for studying the formation and early evolution of super star clusters that are rare in our cosmic backyard. The Sunburst Arc, a lensed Cosmic Noon galaxy, hosts a young super star cluster with escaping Lym
Externí odkaz:
http://arxiv.org/abs/2301.10790
Autor:
Kelly, John M., Hu, Zinan, Takaesu, Felipe, Watanabe, Tatsuya, Storrs, Judd, Blais, Benjamin, Yuhara, Satoshi, Morrison, Adrienne, Nelson, Kirsten, Ulziibayar, Anudari, Heuer, Eric, Anderson, Cole, Jimenez, Michael, Leland, Joseph, Malbrue, Raphael, Arsuaga-Zorrilla, Carmen, Goodchild, Laurie, Naguib, Aymen, McKee, Christopher, Varner, Jordan, DeShetler, Cameron, Spiess, Joshua, Harrison, Andrew, Boe, Brian, Armstrong, Aimee K., Salavitabar, Arash, Hor, Kan, Krishnamurthy, Rajesh, Yates, Andrew R., Shinoka, Toshiharu, Carrillo, Sergio A., Davis, Michael E., Marsden, Alison L., Breuer, Christopher K.
Publikováno v:
In JTCVS Open October 2024 21:268-278
Beginning with cosmological initial conditions at z=100, we simulate the effects of magnetic fields on the formation of Population III stars and compare our results with the predictions of Paper I. We use Gadget-2 to follow the evolution of the syste
Externí odkaz:
http://arxiv.org/abs/2201.02225
Autor:
Li, Pak Shing, Lopez-Rodriguez, Enrique, Ajeddig, Hamza, André, Philippe, McKee, Christopher F., Rho, Jeonghee, Klein, Richard I.
Optical and infrared polarization mapping and recent Planck observations of the filamentary cloud L1495 in Taurus show that the large-scale magnetic field is approximately perpendicular to the long axis of the cloud. We use the HAWC+ polarimeter on S
Externí odkaz:
http://arxiv.org/abs/2111.12864
Publikováno v:
In Journal of Orthopaedics August 2024 54:10-21
A significant fraction of binary neutron star mergers occur in star-forming galaxies where the UV-optical and soft X-ray afterglow emission from the relativistic jet may be absorbed by dust and re-emitted at longer wavelengths. We show that, for merg
Externí odkaz:
http://arxiv.org/abs/2108.04243