Next meeting:
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Votes: 1
3 years ago
Title:
Molecular Gas Reservoirs in Massive Quiescent Galaxies at
$\mathrm{z\sim0.7}$ Linked to Late Time Star Formation
(View PDF)
Author:
Charity Woodrum, Christina C. Williams, Marcia Rieke, Joel Leja, Benjamin D. Johnson, Rachel Bezanson, Robert Kennicutt, Justin Spilker et al.
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3 years ago
Title: ISM metallicity variations across spiral arms in disk galaxies: the impact of local enrichment and g
Link: https://arxiv.org/abs/2209.14576
Description: ISM metallicity variations across spiral arms in disk galaxies: the impact of local enrichment and gas migration in the presence of radial metallicity gradient
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Votes: 1
3 years ago
Title:
Optical Variability of the very Radio-Loud Narrow line Seyfert 1 galaxy,
1H 0323+342
(View PDF)
Author:
Clay S. Turner, Hugh R. Miller, Jeremy D. Maune, Joseph R. Eggen
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Votes: 1
3 years ago
Title:
Rapid Growth of Galactic Supermassive Black Holes through Accreting
Giant Molecular Clouds during Major Mergers of their Host Galaxies
(View PDF)
Author:
Chi-Hong Lin, Ke-Jung Chen, Chorng-Yuan Hwang
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Votes: 1
3 years ago
Title:
Self-gravitating disks around rapidly spinning, tilted black holes:
General relativistic simulations
(View PDF)
Author:
Antonios Tsokaros, Milton Ruiz, Stuart L. Shapiro, Vasileios Paschalidis
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Votes: 1
3 years ago Author:
F. Espinoza-Arancibia, M. Catelan, G. Hajdu, N. Rodríguez-Segovia, G. Boggiano, K. Joachimi, C. Muñoz-López, C. Ordenes-Huanca et al.
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Votes: 1
3 years ago
Title:
BASS. XXXVI. Constraining the Local Supermassive Black Hole - Halo
Connection with BASS DR2 AGN
(View PDF)
Author:
M. C. Powell, S. W. Allen, T. Caglar, N. Cappelluti, F. Harrison, B. E. Irving, M. J. Koss, A. B. Mantz et al.
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Votes: 1
3 years ago Author:
Takahiro Sudoh, John F. Beacom
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3 years ago
Title: Is ozone a reliable proxy for molecular oxygen? I. The O2-O3 relationship for Earth-like atmospheres
Link: https://arxiv.org/abs/2208.09415
Description: Investigating whether O3 can be used as a tracer for O2 in terrestrial exoplanet atmospheres when O2 is not present in detectable levels. Uses models that account for the spectral type of the host star to see how UV radiation would affect the evolution of O3 from O2, and if O3 would serve as a good tracer of atmospheric O2.
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Votes: 1
3 years ago Author:
Erin R. Higgins, Jorick S. Vink, Gautham N. Sabhahit, Andreas A. C. Sander
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