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Akademický článek
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Autor:
Smart, R. L., Bucciarelli, B., Jones, H. R. A., Marocco, F., Andrei, A. H., Goldman, B., Mendez, R. A., d'Avila, V. A., Burningham, B., Camargo, J. I. B., Crosta, M. T., Daprà, M., Jenkins, J. S., Lachaume, R., Lattanzi, M. G., Penna, J. L., Pinfield, D. J., Neto, D. N. da Silva, Sozzetti, A., Vecchiato, A.
Publikováno v:
2018MNRAS.481.3548S
We present new results from the Parallaxes of Southern Extremely Cool dwarfs program to measure parallaxes, proper motions and multi-epoch photometry of L and early T dwarfs. The observations were made on 108 nights over the course of 8 years using t
Externí odkaz:
http://arxiv.org/abs/1811.00672
Autor:
Jarboe, T. R., Benedett, T. E., Everson, C. J., Hansen, C. J., Hossack, A. C., Morgan, K. D., Nelson, B. A., Penna, J. M., Sutherland, D. A.
Self-organization properties of sustained magnetized plasma are applied to selected solar data to understand solar magnetic fields. Torsional oscillations are speed-up and slow-down bands of the azimuthal flow that correlate with the solar cycle, and
Externí odkaz:
http://arxiv.org/abs/1807.09593
Autor:
Jarboe, T. R., Benedett, T. E., Everson, C. J., Hansen, C. J., Hossack, A. C., Morgan, K. D., Nelson, B. A., Penna, J. M., Sutherland, D. A.
The solar dynamo and the solar Global internal Magnetic Structure (GMS) appear to be a thin ($\sim$2 Mm thick) structure near ($\sim$1 Mm below) the solar surface. Evidence for these properties are found from the amplitude of the torsional oscillatio
Externí odkaz:
http://arxiv.org/abs/1712.01247
Autor:
Capotosto S; Department of Orthopedic Surgery, Mount Sinai Hospital, New York, USA., Nazemi AK; Cedars-Sinai Kerlan-Jobe Institute, Los Angeles, California, USA., Komatsu DE; Department of Orthopedics and Rehabilitation, Stony Brook University Hospital, Stony Brook, New York, USA., Penna J; Department of Orthopedics and Rehabilitation, Stony Brook University Hospital, Stony Brook, New York, USA.
Publikováno v:
Orthopaedic journal of sports medicine [Orthop J Sports Med] 2024 Nov 04; Vol. 12 (11), pp. 23259671241275087. Date of Electronic Publication: 2024 Nov 04 (Print Publication: 2024).
Autor:
Marocco, F., Andrei, A. H., Smart, R. L., Jones, H. R. A., Pinfield, D. J., Day-Jones, A. C., Clarke, J. R. A., Sozzetti, A., Lucas, P. W., Bucciarelli, B., Penna, J. L.
We present near-infrared spectroscopy for 52 ultracool dwarfs, including two newly discovered late-M dwarfs, one new late-M subdwarf candidate, three new L and four new T dwarfs. We also present parallaxes and proper motions for 21 of them. Four of t
Externí odkaz:
http://arxiv.org/abs/1309.6525
Autor:
Smart, R. L., Tinney, C. G., Bucciarelli, B., Marocco, F., Abbas, U., Andrei, A., Bernardi, G., Burningham, B., Cardoso, C., Costa, E., Crosta, M. T., Dapra, M., Day-Jones, A., Goldman, B., Jones, H. R. A., Lattanzi, M. G., Leggett, S. K., Lucas, P., Mendez, R., Penna, J. L., Pinfield, D., Smith, L., Sozzetti, A., Vecchiato, A.
The discovery and subsequent detailed study of T dwarfs has provided many surprises and pushed the physics and modeling of cool atmospheres in unpredicted directions. Distance is a critical parameter for studies of these objects to determine intrinsi
Externí odkaz:
http://arxiv.org/abs/1306.4527
Autor:
Andrei, A. H., Souchay, J., Zacharias, N., Smart, R. L., Martins, R. Vieira, Neto, D. N. da Silva, Camargo, J. I. B., Assafin, M., Barache, C., Bouquillon, S., Penna, J. L., Taris, F.
The large number and all-sky distribution of quasars from different surveys, along with their presence in large, deep astrometric catalogs,enables the building of an optical materialization of the ICRS following its defining principles. Namely: that
Externí odkaz:
http://arxiv.org/abs/0907.2403
Publikováno v:
Proceedings of the International Astronomical Union. 08/04/2009, Vol. 5 Issue S264, p49-54. 6p.
Autor:
William B. Seaman
Publikováno v:
Radiology. 90:163-164