Zobrazeno 1 - 10
of 235
pro vyhledávání: '"Rees J. M."'
Autor:
Jacobson-Galan, W. V., Dessart, L., Margutti, R., Chornock, R., Foley, R. J., Kilpatrick, C. D., Jones, D. O., Taggart, K., Angus, C. R., Bhattacharjee, S., Braff, L. A., Brethauer, D., Burgasser, A. J., Cao, F., Carlile, C. M., Chambers, K. C., Coulter, D. A., Dominguez-Ruiz, E., Dickinson, C. B., de Boer, T., Gagliano, A., Gall, C., Gao, H., Gates, E. L., Gomez, S., Guolo, M., Halford, M. R. J., Hjorth, J., Huber, M. E., Johnson, M. N., Karpoor, P. R., Laskar, T., LeBaron, N, Li, Z., Lin, Y., Loch, S. D., Lynam, P. D., Magnier, E. A., Maloney, P., Matthews, D. J., McDonald, M., Miao, H. -Y., Milisavljevic, D., Pan, Y. -C., Pradyumna, S., Ransome, C. L., Rees, J. M., Rest, A., Rojas-Bravo, C., Sandford, N. R., Ascencio, L. Sandoval, Sanjaripour, S., Savino, A., Sears, H., Sharei, N., Smartt, S. J., Softich, E. R., Theissen, C. A., Tinyanont, S., Tohfa, H., Villar, V. A., Wang, Q., Wainscoat, R. J., Westerling, A. L., Wiston, E., Wozniak, M. A., Yadavalli, S. K., Zenati, Y.
We present UV/optical observations and models of supernova (SN) 2023ixf, a type II SN located in Messier 101 at 6.9 Mpc. Early-time ("flash") spectroscopy of SN 2023ixf, obtained primarily at Lick Observatory, reveals emission lines of H I, He I/II,
Externí odkaz:
http://arxiv.org/abs/2306.04721
Publikováno v:
Applied Rheology, Vol 20, Iss 5 (2010)
This paper is concerned with the determination of the constitutive parameters of low concentrations of the complex fluid polyethylene glycol (PEO). Velocity fields of PEO solutions in a microfluidic T-junction have been measured for pressure driven f
Externí odkaz:
https://doaj.org/article/429b2980b7634ba88877462238feb829
Autor:
Marocco, F., Smart, R. L., Mamajek, E. E., Sarro, L. M., Burgasser, A. J., Caballero, J. A., Rees, J. M., Caselden, D., Cruz, K. L., Van Linge, R., Pinfield, D. J.
We present ten new ultra-cool dwarfs in seven wide binary systems discovered using $\textit{Gaia}$ DR2 data, identified as part of our $\textit{Gaia}$ Ultra-Cool Dwarf Sample project. The seven systems presented here include an L1 companion to the G5
Externí odkaz:
http://arxiv.org/abs/2004.04132
Autor:
Milone, A. P., Marino, A. F., Bedin, L. R., Anderson, J., Apai, D., Bellini, A., Dieball, A., Salaris, M., Libralato, M., Nardiello, D., Bergeron, P., Burgasser, A. J., Rees, J. M., Rich, R. M., Richer, H. B.
Historically, multiple populations in Globular Clusters (GCs) have been mostly studied from ultraviolet and optical filters down to stars that are more massive than ~0.6 solar masses. Here we exploit deep near-infrared (NIR) photometry from the Hubbl
Externí odkaz:
http://arxiv.org/abs/1901.07230
Autor:
Mens, D. M.1 (AUTHOR) d.mens@erasmusmc.nl, van Rees, J. M.1 (AUTHOR), Wilting, S. M.1 (AUTHOR), Verhoef, C.1 (AUTHOR)
Publikováno v:
BMC Cancer. 12/4/2023, Vol. 23 Issue 1, p1-6. 6p.
Publikováno v:
E. E. Mamajek et al. (2018) Res. Notes AAS 2 205
While spectroscopically characterizing nearby ultracool dwarfs discovered in the Gaia Second Data Release with the TripleSpec spectrograph on the Palomar 200'' telescope, we encountered a particularly cool, nearby, new member of the solar neighborhoo
Externí odkaz:
http://arxiv.org/abs/1811.03477
Autor:
Libralato, M., Bellini, A., Bedin, L. R., Moreno, E., Fernández-Trincado, J. G., Pichardo, B., van der Marel, R. P., Anderson, J., Apai, D., Burgasser, A. J., Marino, A. F., Milone, A. P., Rees, J. M., Watkins, L. L.
In this paper we report a new estimate of the absolute proper motion (PM) of the globular cluster NGC 5139 ($\omega$ Cen) as part of the HST large program GO-14118+14662. We analyzed a field 17 arcmin South-West of the center of $\omega$ Cen and comp
Externí odkaz:
http://arxiv.org/abs/1801.01502
Autor:
Bellini, A., Libralato, M., Bedin, L. R., Milone, A. P., van der Marel, R. P., Anderson, J., Apai, D., Burgasser, A. J., Marino, A. F., Rees, J. M.
In this second installment of the series, we look at the internal kinematics of the multiple stellar populations of the globular cluster $\omega$ Centauri in one of the parallel Hubble Space Telescope (HST) fields, located at about 3.5 half-light rad
Externí odkaz:
http://arxiv.org/abs/1801.01504
Autor:
Milone, A. P., Marino, A. F., Bedin, L. R., Anderson, J., Apai, D., Bellini, A., Bergeron, P., Burgasser, A. J., Dotter, A., Rees, J. M.
As part of a large investigation with Hubble Space Telescope to study the faintest stars within the globular cluster Omega Centauri, in this work we present early results on the multiplicity of its main sequence (MS) stars, based on deep optical and
Externí odkaz:
http://arxiv.org/abs/1704.00418
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.