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pro vyhledávání: '"Milky Way Galaxy"'
We analyse the energy spectral density properties of Gravitational waves from Galactic binary populations in the~\text{mHz} band targeted by the Laser Interferometer Space Antenna mission. Our analysis is based on combining BPASS with a Milky Way ana
Externí odkaz:
http://arxiv.org/abs/2411.02563
Autor:
Lian, Jianhui, Zasowski, Gail, Chen, Bingqiu, Imig, Julie, Wang, Tao, Boardman, Nicholas, Liu, Xiaowei
The size of a galaxy is one of the fundamental parameters that reflects its growth and assembly history. Traditionally, the size of the Milky Way has been characterized by the scale length of the disk, based on the assumption of an exponential densit
Externí odkaz:
http://arxiv.org/abs/2406.05604
Autor:
Mishenina, T., Pignatari, M., Usenko, I., Soubiran, C., Thielemann, F. -K., Kniazev, A. Yu., Korotin, S. A., Gorbaneva, T.
The oldest stars in the Milky Way are metal-poor with [Fe/H] < -- 1.0, displaying peculiar elemental abundances compared to solar values. The relative variations in the chemical compositions among stars is also increasing with decreasing stellar meta
Externí odkaz:
http://arxiv.org/abs/2405.11234
The Milky Way galaxy is estimated to be home to ten million to a billion stellar-mass black holes (BHs). Accurately determining this number and distribution of BH masses can provide crucial information about the processes involved in BH formation, th
Externí odkaz:
http://arxiv.org/abs/2401.02790
We explore the influence of the Milky Way galaxy's chemical evolution on the formation, structure, and habitability of the Solar system. Using a multi-zone Galactic Chemical Evolution (GCE) model, we successfully reproduce key observational constrain
Externí odkaz:
http://arxiv.org/abs/2310.10335
Autor:
Deel, Gary L.
Publikováno v:
Space Education & Strategic Applications. 2024, Vol. 4 Issue 3, p89-92. 4p.
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