The DOI matches its Crossref record; 233 of the 233 references it cites were found in a registry or an index.
Accurate distances to Galactic globular clusters through a combination of Gaia EDR3, HST, and literature data
Open accessAbstract
We have derived accurate distances to Galactic globular clusters by combining data from the Gaia Early Data Release 3 (EDR3) with distances based on Hubble Space Telescope (HST) data and literature-based distances. We determine distances either directly from the Gaia EDR3 parallaxes, or kinematically by combining line-of-sight velocity dispersion profiles with Gaia EDR3 and HST-based proper motion velocity dispersion profiles. We furthermore calculate cluster distances from fitting nearby subdwarfs, whose absolute luminosities we determine from their Gaia EDR3 parallaxes, to globular cluster main sequences. We finally use HST-based stellar number counts to determine distances. We find good agreement in the average distances derived from the different methods down to a level of about 2 per cent. Combining all available data, we are able to derive distances to 162 Galactic globular clusters, with the distances to about 20 nearby globular clusters determined with an accuracy of 1 per cent or better. We finally discuss the implications of our distances for the value of the local Hubble constant.
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Cites
Gaia Collaboration, Prusti, T., de Bruijne, J. H. J., Brown, A. G. A., Vallenari, A., Babusiaux, C., Bailer-Jones, C. A. L., Bastian, U., Biermann, M., Evans, D. W., et al. (2016) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201629272 · Cited by 6,946
A Catalog of Parameters for Globular Clusters in the Milky Way
Harris, W. E. (1996) · The Astronomical Journal · doi:10.1086/118116 · Cited by 4,500 · cited 2×
“To create the isochrones, we use the cluster ages derived by VandenBerg et al. (2013), or, for clusters not studied by them, from available literature sources, and take the cluster metallicities and reddenings from Harris (1996).”
MethodBressan, A., Marigo, P., Girardi, L., Salasnich, B., Dal Cero, C., Rubele, S., & Nanni, A. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21948.x · Cited by 4,174
Riess, A. G., Casertano, S., Yuan, W., Macri, L. M., & Scolnic, D. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab1422 · Cited by 1,986
Tensions between the early and late Universe
Verde, L., Treu, T., & Riess, A. G. (2019) · Nature Astronomy · doi:10.1038/s41550-019-0902-0 · Cited by 1,380
Sirianni, M., Jee, M. J., Benítez, N., Blakeslee, J. P., Martel, A. R., Meurer, G., Clampin, M., De Marchi, G., Ford, H. C., Gilliland, R., et al. (2005) · Publications of the Astronomical Society of the Pacific · doi:10.1086/444553 · Cited by 1,091
Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position
Lindegren, L., Bastian, U., Biermann, M., Bombrun, A., de Torres, A., Gerlach, E., Geyer, R., Hernández, J., Hilger, T., Hobbs, D., et al. (2021) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202039653 · Cited by 1,024
Dynamical evolution of star clusters in tidal fields
Baumgardt, H., & Makino, J. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06286.x · Cited by 773
Self-citationAn absolutely calibrated Teffscale from the infrared flux method: Dwarfs and subgiants
Casagrande, L., Ramírez, I., Meléndez, J., Bessell, M., & Asplund, M. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913204 · Cited by 718
A Gaia DR2 view of the open cluster population in the Milky Way
Cantat-Gaudin, T., Jordi, C., Vallenari, A., Bragaglia, A., Balaguer-Núñez, L., Soubiran, C., Bossini, D., Moitinho, A., Castro-Ginard, A., Krone-Martins, A., et al. (2018) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201833476 · Cited by 700
Cited by
Measurements of the Hubble Constant: Tensions in Perspective
Freedman, W. L. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac0e95 · Cited by 577
Koposov, S. E., Erkal, D., Li, T. S., Da Costa, G. S., Cullinane, L. R., Ji, A. P., Kuehn, K., Lewis, G. F., Pace, A. B., Shipp, N., et al. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad551 · Cited by 109
Metadata
- Authors
- Baumgardt, H., & Vasiliev, E.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2021-05-24
- Volume
- 505
- Issue
- 4
- Pages
- 5957-5977
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W3163513588
- Cited by
- 369
- References
- 233
- FWCI
- 31.61
- Type
- journal article
- Language
- en
- Open access
- green
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- Baumgardt, H., & Vasiliev, E. (2021). Accurate distances to Galactic globular clusters through a combination of Gaia EDR3, HST, and literature data. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/stab1474
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