https://www.astronomy.com/science/astronomers-explain-why-disk-galaxies-eventually-look-alike/
Astronomers explain why disk galaxies eventually look alike | Astronomy.com
May 18, 2023 - Researchers indicate that the key to the smooth, steady fade of older disk galaxies is clumps of interstellar gases and new stars within young galaxy disks.
disk galaxieslook alikeastronomersexplaineventually
https://www.astronomy.com/science/all-disk-galaxies-rotate-once-every-billion-years/
All disk galaxies rotate once every billion years
May 18, 2023 - In a study published March 14 in The Monthly Notices of the Royal Astronomical Society, astronomers announced the discovery that all galaxies rotate about once...
disk galaxiesrotateeverybillionyears
https://iac.es/en/science-and-technology/publications/disk-galaxies-are-self-similar-universality-h-i-halo-mass-ratio-isolated-disks?base_route_name=entity.node.canonical&overridden_route_name=entity.node.canonical&page_manager_page=node_view&page_manager_page_variant=node_view-panels_variant-15&page_manager_page_variant_weight=-6
Disk Galaxies Are Self-similar: The Universality of the H I-to-Halo Mass Ratio for Isolated Disks |...
Observed scaling relations in galaxies between baryons and dark matter global properties are key to shed light on the process of galaxy formation and on the...
https://www.aanda.org/articles/aa/abs/2001/24/aa1314/aa1314.html
Modeling the spectral energy distribution of galaxies - II. Disk opacity and star formation in 5...
https://www.aanda.org/articles/aa/abs/2007/24/aa7599-07/aa7599-07.html
Fueling the central engine of radio galaxies - I. The molecular/dusty disk of 4C 31.04 | Astronomy...
https://www.aanda.org/articles/aa/ref/2010/07/aa12566-09/aa12566-09.html
The dark matter halo shape of edge-on disk galaxies - II. Modelling the HI observations: methods |...
https://iac.es/es/ciencia-y-tecnologia/publicaciones/disk-galaxies-are-self-similar-universality-h-i-halo-mass-ratio-isolated-disks?base_route_name=entity.node.canonical&overridden_route_name=entity.node.canonical&page_manager_page=node_view&page_manager_page_variant=node_view-panels_variant-15&page_manager_page_variant_weight=-6
Disk Galaxies Are Self-similar: The Universality of the H I-to-Halo Mass Ratio for Isolated Disks |...
Observed scaling relations in galaxies between baryons and dark matter global properties are key to shed light on the process of galaxy formation and on the...
https://arxiv.org/abs/2211.00036
[2211.00036] The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk...
Abstract page for arXiv paper 2211.00036: The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
https://www.aanda.org/articles/aa/ref/2025/07/aa47922-23/aa47922-23.html
Dark matter fraction in disk-like galaxies over the past 10 Gyr | Astronomy & Astrophysics (A&A)
https://www.aanda.org/articles/aa/ref/2023/03/aa42581-21/aa42581-21.html
ISM metallicity variations across spiral arms in disk galaxies - The impact of local enrichment and...
https://arxiv.org/abs/0711.4995
[0711.4995] Vigorous star formation with low efficiency in massive disk galaxies at z=1.5
Abstract page for arXiv paper 0711.4995: Vigorous star formation with low efficiency in massive disk galaxies at z=1.5
https://www.iac.es/en/science-and-technology/publications/disk-galaxies-are-self-similar-universality-h-i-halo-mass-ratio-isolated-disks?overridden_route_name=entity.node.canonical&base_route_name=entity.node.canonical&page_manager_page=node_view&page_manager_page_variant=node_view-panels_variant-15&page_manager_page_variant_weight=-6
Disk Galaxies Are Self-similar: The Universality of the H I-to-Halo Mass Ratio for Isolated Disks |...
Observed scaling relations in galaxies between baryons and dark matter global properties are key to shed light on the process of galaxy formation and on the...
https://www.aanda.org/articles/aa/ref/2002/22/aa2193/aa2193.html
Position-velocity diagrams of ionized gas in the inner regions of disk galaxies | Astronomy &...
https://www.aanda.org/articles/aa/abs/2016/11/aa29115-16/aa29115-16.html
Automated bar detection in local disk galaxies from the SDSS - The colors of bars | Astronomy &...
https://www.aanda.org/articles/aa/full_html/2017/01/aa28895-16/aa28895-16.html
Modelling resonances and orbital chaos in disk galaxies - Application to a Milky Way spiral model |...
https://www.iac.es/es/ciencia-y-tecnologia/congresos-y-charlas/charlas/1-understanding-formation-central-regions-disk-galaxies-2-high-angular?base_route_name=entity.node.canonical&overridden_route_name=entity.node.canonical&page_manager_page=node_view&page_manager_page_variant=node_view-panels_variant-17&page_manager_page_variant_weight=0
(1) Understanding the formation of the central regions of disk galaxies (2) High angular resolution...
(1) In the last decades, numerous exoplanetary systems have been detected and studied with different techniques. Obtaining direct images of such systems is...
https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/sfr-bulgetodisk-ratios-from-the-califa-ifs-nearby-galaxies-survey/0889C11C2D0F1AE61CBDA7453FC087A8
SFR bulge-to-disk ratios from the CALIFA IFS nearby galaxies survey | Proceedings of the...
SFR bulge-to-disk ratios from the CALIFA IFS nearby galaxies survey - Volume 11 Issue S315
https://www.aanda.org/articles/aa/abs/2001/08/aa10099/aa10099.html
Optical surface photometry of a sample of disk galaxies - II. Structural components | Astronomy &...
a sample
https://www.aanda.org/articles/aa/abs/2008/39/aa09407-08/aa09407-08.html
Bulges of disk galaxies at intermediate redshifts - II. Nuclear, disk, and global colors in the...