Zobrazeno 1 - 10
of 2 188
pro vyhledávání: '"Parisi M"'
Publikováno v:
A&A 689, A115 (2024)
The VISTA Variables in the Via L\'actea Extended Survey (VVVX) enables exploration of previously uncharted territories within the inner Milky Way (MW), particularly those obscured by stellar crowding and intense extinction. Our objective is to identi
Externí odkaz:
http://arxiv.org/abs/2406.09216
Publikováno v:
Cancer Management and Research, Vol Volume 10, Pp 249-256 (2018)
Reshma L Mahtani,1 Monika Parisi,2 Stefan Glück,3 Quanhong Ni,2 Siyeon Park,4 Corey Pelletier,2 Claudio Faria,2 Fadi Braiteh5,6 1Division of Hematology/Oncology, University of Miami, Miami, FL, 2Health Economics and Outcomes Research, Celgene Corpor
Externí odkaz:
https://doaj.org/article/9ef32653c5ae444f91d95b9b26fcce42
Autor:
Parisi, M. C., Oliveira, R. A. P., Angelo, M., Dias, B., Maia, F., Saroon, S., Feinstein, C., Santos Jr., J. F. C., Bica, E., Ferreira, B. Pereira Lima, Fernández-Trincado, J. G., Westera, P., Minniti, D., Garro, E. R., Santrich, O. J. Katime, De Bortoli, B., Souza, S., Kerber, L., Pérez-Villegas, A.
The structure of the Small Magellanic Cloud (SMC) outside of its main body is characterised by tidal branches resulting from its interactions mainly with the Large Magellanic Cloud (LMC). Characterising the stellar populations in these tidal componen
Externí odkaz:
http://arxiv.org/abs/2312.09756
Publikováno v:
Cancer Management and Research, Vol Volume 9, Pp 141-148 (2017)
Fadi Braiteh,1 Manish B Patel,2 Monika Parisi,2 Quanhong Ni,2 Siyeon Park,2,3 Claudio Faria2 1Comprehensive Cancer Centers of Nevada, University of Nevada School of Medicine, Las Vegas, NV, 2Celgene Corporation, Summit, NJ, 3The Ohio State University
Externí odkaz:
https://doaj.org/article/86965f172423499db78fa51ca523c31d
Autor:
Saroon, S., Dias, B., Tsujimotto, T., Parisi, M. C., Maia, F., Kerber, L., Bekki, K., Minniti, D., Oliveira, R. A. P., Westera, P., Santrich, O. J. K., Bica, E., Sanmartim, D., Quint, B. C., Fraga, L.
Publikováno v:
A&A 677, A35 (2023)
The chemical evolution history of the Small Magellanic Cloud (SMC) has been a matter of debate for decades. The challenges in understanding the SMC chemical evolution are related to a very slow star formation rate (SFR) combined with bursts triggered
Externí odkaz:
http://arxiv.org/abs/2307.08709
Autor:
Oliveira, R. A. P., Maia, F. F. S., Barbuy, B., Dias, B., Santos Jr., J. F. C., Souza, S. O., Kerber, L. O., Bica, E., Sanmartim, D., Quint, B., Fraga, L., Armond, T., Minniti, D., Parisi, M. C., Santrich, O. J. Katime, Angelo, M. S., Pérez-Villegas, A., De Bórtoli, B. J.
The formation scenario of the Magellanic Bridge during an encounter between the Large and Small Magellanic Clouds $\sim200\,$Myr ago, as proposed by $N$-body models, would be imprinted in the chemical enrichment and kinematics of its stars, and sites
Externí odkaz:
http://arxiv.org/abs/2306.05503
Publikováno v:
International Journal of Nephrology and Renovascular Disease, Vol 2015, Iss default, Pp 59-64 (2015)
Chrysoula Pipili,1 Eirini Grapsa,1 Elli-Sophia Tripodaki,1 Sophia Ioannidou,2 Christos Manetos,1 Maria Parisi,1 Serafim Nanas1 1First Critical Care Department, 2Laboratory of Biochemistry, Evangelismos General Hospital, National and Kapodistrian Univ
Externí odkaz:
https://doaj.org/article/f29a2e4c3d9448f4b62306cc6b9c3a57
Autor:
Rodríguez, M. Jimena, Feinstein, C., Baume, G., Dias, B., Maia, F. S. M., Santos Jr., J. F. C., Kerber, L., Minniti, D., Pérez-Villegas, A., De Bórtoli, B., Parisi, M. C., Oliveira, R. A. P.
We present a study of the internal structure of 82 star clusters located at the outer regions of the Large Magellanic Cloud and the Small Magellanic Cloud using data of the VISCACHA Survey. Through the construction of the minimum spanning tree, which
Externí odkaz:
http://arxiv.org/abs/2212.09685
Autor:
Geisler, D., Parisi, M. C., Dias, B., Villanova, S., Mauro, F., Saviane, I., Cohen, R. E., Bidin, C. Moni, Minniti, D.
Publikováno v:
A&A 669, A115 (2023)
Globular clusters (GCs) are excellent tracers of the formation and early evolution of the Milky Way. The bulge GCs (BGCs) are particularly important because they can reveal vital information about the oldest, in-situ component of the Milky Way. We ai
Externí odkaz:
http://arxiv.org/abs/2210.02193
Autor:
Bica, E., Maia, F. F. S., Oliveira, R. A. P., Dias, B., Santos Jr., J. F. C., Rocha, J. P., Kerber, L., Gardin, J. F., Armond, T., Parisi, M. C., Souza, S. O., Barbuy, B.
We present the analysis of three faint clusters of the Small Magellanic Cloud RZ82, HW42 and RZ158. We employed the SOAR telescope instrument SAM with adaptive optics, allowing us to reach to V~23-24 mag, unprecedentedly, a depth sufficient to measur
Externí odkaz:
http://arxiv.org/abs/2209.05532