Results 81 to 90 of about 104,909 (264)

Lactea: Web‐Based Spectrum‐Preserving Multi‐Resolution Visualization of the GAIA Star Catalog

Computer Graphics Forum, EarlyView.
Abstract The explosion of data in astronomy has resulted in an era of unprecedented opportunities for discovery. The GAIA mission's catalog, containing a large number of light sources (mostly stars) with several parameters such as sky position and proper motion, is playing a significant role in advancing astronomy research and has been crucial in ...
Reem Alghamdi, Markus Hadwiger, Guido Reina, Alberto Jaspe‐Villanueva   +3 more
wiley   +1 more source

Tracing the first stars and galaxies of the Milky Way [PDF]

Monthly Notices of the Royal Astronomical Society, 2017
We use 30 high-resolution dark matter halos of the $Caterpillar$ simulation suite to probe the first stars and galaxies of Milky Way-mass systems. We quantify the environment of the high-$z$ progenitors of the Milky Way and connect them to the properties of the host and satellites today.
Alexander P. Ji, Facundo A. Gómez, Brendan F. Griffen, Gregory A. Dooley, Anna Frebel, Brian W. O'Shea, Brian W. O'Shea   +6 more
openaire   +5 more sources

Milky Way Satellite Census. II. Galaxy–Halo Connection Constraints Including the Impact of the Large Magellanic Cloud [PDF]

Astrophysical Journal, 2019
The population of Milky Way (MW) satellites contains the faintest known galaxies and thus provides essential insight into galaxy formation and dark matter microphysics.
E. Nadler, Risa Wechsler, K. Bechtol, Yao-Yuan Mao, Yao-Yuan Mao, G. Green, A. Drlica-Wagner, A. Drlica-Wagner, M. McNanna, S. Mau, A. Pace, A. Pace, J. Simon, A. Kravtsov, S. Dodelson, Tian Li, A. Riley, Mei-Yu Wang, T. Abbott, M. Aguena, S. Allam, J. Annis, S. Ávila, G. Bernstein, E. Bertin, E. Bertin, D. Brooks, D. Burke, A. Rosell, M. Kind, J. Carretero, M. Costanzi, L. Costa, J. Vicente, S. Desai, A. Evrard, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztañaga, D. Gerdes, D. Gruen, J. Gschwend, G. Gutiérrez, W. Hartley, W. Hartley, S. Hinton, K. Honscheid, E. Krause, K. Kuehn, K. Kuehn, N. Kuropatkin, O. Lahav, M. Maia, J. Marshall, F. Menanteau, R. Miquel, A. Palmese, F. Paz-Chinchón, A. Plazas, A. Romer, E. Sánchez, B. Santiago, V. Scarpine, S. Serrano, M. Smith, M. Soares-Santos, E. Suchyta, G. Tarlé, D. Thomas, T. Varga, T. Varga, A. Walker   +73 more
semanticscholar   +1 more source

What Does the Milky Way Look Like?

The Astrophysical Journal, 2023
In spite of much work, the overall spiral structure morphology of the Milky Way remains somewhat uncertain. In the last two decades, accurate distance measurements have provided us with an opportunity to solve this issue.
Y. Xu, C. J. Hao, D. J. Liu, Z. H. Lin, S. B. Bian, L. G. Hou, J. J. Li, Y. J. Li   +7 more
doaj   +1 more source

Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties

The Astrophysical Journal
Very metal-poor (VMP) stars record the signatures of early accreted galaxies, making them essential tools for unraveling the early stages of Galaxy formation.
Ruizhi Zhang, Tadafumi Matsuno, Haining Li, Wako Aoki, Xiang-Xiang Xue, Takuma Suda, Gang Zhao, Yuqin Chen, Miho N. Ishigaki, Jianrong Shi, Qianfan Xing, Jingkun Zhao   +11 more
doaj   +1 more source

4MOST Consortium Survey 3: Milky Way Disc and Bulge Low-Resolution Survey (4MIDABLE-LR)

, 2019
The mechanisms of the formation and evolution of the Milky Way are encoded in the orbits, chemistry and ages of its stars. With the 4MOST MIlky way Disk And BuLgE Low-Resolution Survey (4MIDABLE-LR) we aim to study kinematic and chemical substructures in
Anders, F., Andrae, R., Arentsen, A., Asplund, M., Bensby, T., Bergemann, M., Casagrande, L., Cescutti, G., Chiappini, C., Church, R., Feltzing, S., Fouesneau, M., Fusillo, N., Gerhard, O., Grebel, E., Guiglion, G., Khalatyan, A., Kordopatis, G., Kovalev, M., Lemasle, B., Matijevic, G., McMillan, P., Minchev, I., Monari, G., Queiroz, A., Rix, H., Rybizki, J., Ryde, N., Schwope, A., Starkenburg, E., Steinmetz, M., Storm, J., Team, 4., Traven, G., Tremblay, P., Valentini, M., Walton, N., Xiang, M., Zucker, D.   +38 more
core   +1 more source

Spaceborne and spaceborn: Physiological aspects of pregnancy and birth during interplanetary flight

Experimental Physiology, EarlyView.
Abstract Crewed interplanetary return missions that are on the planning horizon will take years, more than enough time for initiation and completion of a pregnancy. Pregnancy is viewed as a sequence of processes – fertilization, blastocyst formation, implantation, gastrulation, placentation, organogenesis, gross morphogenesis, birth and neonatal ...
Arun V. Holden
wiley   +1 more source

The Three-phase Evolution of the Milky Way

The Astrophysical Journal
We illustrate the formation and evolution of the Milky Way over cosmic time, utilizing a sample of 10 million red giant stars with full chemodynamical information, including metallicities and α -abundances from low-resolution Gaia XP spectra.
Vedant Chandra, Vadim A. Semenov, Hans-Walter Rix, Charlie Conroy, Ana Bonaca, Rohan P. Naidu, René Andrae, Jiadong Li, Lars Hernquist   +8 more
doaj   +1 more source

(2R,6R)‐hydroxynorketamine prevents opioid abstinence‐related negative affect and stress‐induced reinstatement in mice

British Journal of Pharmacology, Volume 182, Issue 15, Page 3428-3451, August 2025.
Abstract Background and Purpose Opioid use disorder (OUD) is a pressing public health concern marked by frequent relapse during periods of abstinence, perpetuated by negative affective states. Classical antidepressants or the currently prescribed opioid pharmacotherapies have limited efficacy to reverse the negative affect or prevent relapse ...
Andria Michael, Anna Onisiforou, Polymnia Georgiou, Morfeas Koumas, Chris Powels, Elmar Mammadov, Andrea N. Georgiou, Panos Zanos   +7 more
wiley   +1 more source

Impact of Fatty Acid Carbon Chain Length and Protein Composition on Physicochemical and Digestive Properties of MFGM Contained Emulsions

Food Science &Nutrition, Volume 13, Issue 7, July 2025.
Emulsions prepared by OPO (long‐chain fatty acids) exhibited the largest average particle size and greater stability compared to those with medium‐chain fat (coconut oil) and ultra‐long‐chain fat (DHA algae oil). When whey protein and casein were added in a 6:4 ratio, the effect of fatty acid carbon chain length on the average particle and the ...
Yanchen Liu, Ning Wang, Yunpeng Xu, Zihao Guo, Guangqing Mu, Xuemei Zhu   +5 more
wiley   +1 more source