This page lists the papers that result from the research proejcts carried out within MWGaiaDN.
ESR led papers
- Clues to growth and disruption of two neighbouring spiral arms of the Milky Way
Natsuki Funakoshi, Noriyuki Matsunaga, Daisuke Kawata, Junichi Baba, Daisuke Taniguchi, Michiko Fujii, 2024, MNRAS 533, 4324
ADS - Thick-to-thin disc transition and gas disc shrinking induced by the Gaia-Sausage-Enceladus merger
Natsuki Funakoshi, Daisuke Kawata, Jason L. Sanders, Ioana Ciucă, Robert J. J. Grand, HanYuan Zhāng, 2025, MNRAS 543, 2275
ADS - Asymmetries in the LMC velocity maps
M. Schölch, Ó. Jiménez-Arranz, M. Romero-Gómez, X. Luri, D. Hobbs, D. Salmerón-Larraz, M. López Vilamajó, 2025, A&A 701, A227
ADS - Modelling the Milky Way’s exoplanet population based on cosmological galaxy simulations
Chloé Padois, Daniel del Ser, Friedrich Anders, João A. S. Amarante, Hélio D. Perottoni, Thomas Hajnik, Diogo Souto, Nayara I. Feliciano-Souza, Daisuke Kawata, Eder Martioli, 2025, A&A accepted,
Other papers
- Growing local arm inferred by the breathing motion
Asano T., Kawata D., Fujii M., Baba, J. 2024, MNRAS 529, L7
ADS - The impact of bar origin and morphology on stellar migration
Iles E. J., Pettitt A. R., Okamoto T., Kawata D., 2024 MNRAS 527, 2799
ADS - Impacts of the Local arm on the local circular velocity inferred from the Gaia DR3 young stars in the Milky Way
Almannaei A. S., Kawata D., Baba J., Hunt J. A. S., Seabroke G., Yan Z., 2024, MNRAS 529, 1035
ADS - The epoch of the Milky Way’s bar formation: dynamical modelling of Mira variables in the nuclear stellar disc
Sanders J. L., Kawata D., Matsunaga N., Sormani M. C., Smith L. C., Minniti D., Gerhard O., 2024, MNRAS 530, 2297
ADS - On the Age Distribution of Classical Cepheids in the Galaxy
Anders F., Padois C., Vilanova Sar M., Semczuk M., del Alcázar-Julià M., Figueras F., 2025, Astronomische Nachrichten, Volume 346, Issue 5, e70009
ADS