Zobrazeno 1 - 10
of 296
pro vyhledávání: '"Franz O"'
Publikováno v:
Journal of Pediatric Surgery Case Reports, Vol 30, Iss C, Pp 86-89 (2018)
Externí odkaz:
https://doaj.org/article/2566f460573d40cf82f138963597f545
Autor:
Gazivoda, Victor P., Koshenkov, Vadim P., Kangas-Dick, Aaron W., Greenbaum, Alissa, Davis, Catherine, Smith, Franz O., Hilden, Patrick D., Berger, Adam C.
Publikováno v:
In Journal of Surgical Research September 2023 289:253-260
Autor:
Faller, Lisa-Marie, Deniz Varsavas, Sakine, M. J. Ali, Ahmed, Michalec, Pawel, Lakshmi Gidugu, Srinivas, Spintzyk, Sebastian, Riemelmoser, Franz O.
Publikováno v:
In Materials Today: Proceedings 2022 70:512-518
Autor:
Benedict, G. F., Henry, T. J., Franz, O. G., McArthur, B. E., Wasserman, L. H., Jao, Wei-Chun, Cargile, P. A., Dieterich, S. B., Bradley, A. J., Nelan, E. P., Whipple, A. L.
We present a Mass-Luminosity Relation (MLR) for red dwarfs spanning a range of masses from 0.62 Msun to the end of the stellar main sequence at 0.08 Msun. The relation is based on 47 stars for which dynamical masses have been determined, primarily us
Externí odkaz:
http://arxiv.org/abs/1608.04775
Autor:
Simon, M., Schaefer, G. H., Prato, L., Ruiz-Rodriguez, Dary, Karnath, N., Franz, O. G., Wasserman, L. H.
As part of our continuing campaign to measure the masses of pre-main sequence stars dynamically and thus to assess the reliability of the discrepant theoretical calculations of contraction to the main sequence, we present new results for NTTS 045251+
Externí odkaz:
http://arxiv.org/abs/1306.4393
Autor:
Victor P. Gazivoda, Vadim P. Koshenkov, Aaron W. Kangas-Dick, Alissa Greenbaum, Catherine Davis, Franz O. Smith, Patrick D. Hilden, Adam C. Berger
Publikováno v:
Journal of Surgical Research. 289:253-260
Autor:
Coups, Elliot J., Manne, Sharon L., Ohman Strickland, Pamela, Hilgart, Michelle, Goydos, James S., Heckman, Carolyn J., Chamorro, Paola, Rao, Babar K., Davis, Moira, Smith, Franz O., Thorndike, Frances P., Ritterband, Lee M.
Publikováno v:
In Contemporary Clinical Trials August 2019 83:117-127
The young system RX J0529.3+1210 was initially identified as a single-lined spectroscopic binary. Using high-resolution infrared spectra, acquired with NIRSPEC on Keck II, we measured radial velocities for the secondary. The method of using the infra
Externí odkaz:
http://arxiv.org/abs/0808.3602
Autor:
Patience, J., Zavala, R. T., Prato, L., Franz, O., Wasserman, L., Tycner, C., Hutter, D. J., Hummel, C. A.
With the Navy Prototype Optical Interferometer (NPOI), the binary system Theta 1 Orionis C, the most massive member of the Trapezium, was spatially resolved over a time period extending from February 2006 to March 2007. The data show significant orbi
Externí odkaz:
http://arxiv.org/abs/0801.2584
Autor:
Boden, A. F., Sargent, A. I., Akeson, R. L., Carpenter, J. M., Torres, G., Latham, D. W., Soderblom, D. R., Nelan, E., Franz, O. G., Wasserman, L. H.
Publikováno v:
Astrophys.J.635:442-451,2005
We report on Keck Interferometer observations of the double-lined binary (B) component of the quadruple pre-main sequence (PMS) system HD 98800. With these interferometric observations combined with astrometric measurements made by the Hubble Space T
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508331