Zobrazeno 1 - 10
of 24 574
pro vyhledávání: '"galactic disk"'
Open clusters (OCs) in the Galaxy are excellent probes for tracing the structure and evolution of the Galactic disk. We present an updated catalog of parameters for 1,145 OCs, estimated using the Gaia DR3 data earlier listed in Cantat-Gaudin et al. (
Externí odkaz:
http://arxiv.org/abs/2410.15305
The bulk of old stars in the Galactic disk have migrated radially by up to several kpc in their lifetimes, yet the disk has remained relatively cool, i.e., the ratio of radial heating to migration has been small. Here, we demonstrate that this small
Externí odkaz:
http://arxiv.org/abs/2411.08944
Autor:
Albarracín, Rogelio, Zoccali, M., Carvajal, J. Olivares, Rojas-Arriagada, Á., Minniti, J. H., Catelan, M., De Leo, M., Gran, F., Ramos, R. Contreras, Navarro, Á. Valenzuela, Salvo-Guajardo, C.
The structure and kinematics of the Milky Way disk are largely inferred from the solar vicinity. To gain a comprehensive understanding, it is essential to find reliable tracers in less-explored regions like the bulge and the far side of the disk. Mir
Externí odkaz:
http://arxiv.org/abs/2411.04623
Using nearly 230,000 red clump stars selected from LAMOST and Gaia, we conduct a comprehensive analysis of the stellar age-velocity dispersion relations (AVRs) for various disk populations, within 5.0 $\leq$ $R$ $\leq$ 15.0 kpc and $|Z|$ $\leq$ 3.0 k
Externí odkaz:
http://arxiv.org/abs/2412.07089
Publikováno v:
Astrobiology, 24, 10, e916 2024
In Lammer et al. 2024, we defined Earth-like Habitats (EH) as rocky planets in the habitable zone of complex life (HZCL) on which Earth-like N$_2$-O$_2$-dominated atmospheres with minor amounts of CO$_2$ can exist and derived a formula for estimating
Externí odkaz:
http://arxiv.org/abs/2412.05002
We investigate the nature of star formation in gas-rich galaxies at $z > 7$ forming in a markedly overdense region, in the whereabouts of a massive virialized halo already exceeding $10^{12}$ M$_{\odot}$. We find that not only the primary galaxy, but
Externí odkaz:
http://arxiv.org/abs/2411.00670
The Galactic disk is one of the main components of the Milky Way, which contributes most of the luminosity. Its structure is essential for understanding the formation and evolution of the Milky Way. Using 174,443 K-type dwarf stars observed by both L
Externí odkaz:
http://arxiv.org/abs/2407.09312
Publikováno v:
A&A 690, A107 (2024)
Stellar ages are an important parameter to study the chemical evolution of the Galaxy. In recent years, several studies have established the existence of a relationship between chemical clocks and stellar ages. The [Y/Mg] clock is a promising techniq
Externí odkaz:
http://arxiv.org/abs/2407.07283
Autor:
Mondal, Samaresh, Ponti, Gabriele, Filor, Luke, Bao, Tong, Haberl, Frank, Salcedo, Ciro, Campana, Sergio, Hailey, Charles J., Mori, Kaya, Rea, Nanda
Publikováno v:
A&A 689, A172 (2024)
We aim at characterizing the population of low-luminosity X-ray sources in the Galactic plane by studying their X-ray spectra and periodic signals in the light curves. We are performing an X-ray survey of the Galactic disk using XMM-Newton, and the s
Externí odkaz:
http://arxiv.org/abs/2407.03025
Previous studies have revealed that the Galactic warp is a long-lived, nonsteady, and asymmetric structure. There is a need for a model that accounts for the warp's long-term evolution. Given that this structure has persisted for over 5 Gyrs, its tim
Externí odkaz:
http://arxiv.org/abs/2409.03264