Zobrazeno 1 - 10
of 113
pro vyhledávání: '"Hamilton, R. T."'
Autor:
Lopez-Rodriguez, E., Dowell, C. D., Jones, T. J., Harper, D. A., Berthoud, M., Chuss, D., Dale, D. A., Guerra, J. A., Hamilton, R. T., Looney, L. W., Michail, J. M., Nikutta, R., Novak, G., Santos, F. P., Sheth, K., Siah, J., Staguhn, J., Stephens, I. W., Tassis, K., Trinh, C. Q., Ward-Thompson, D., Werner, M., Wollack, E. J., Zweibel, E.
We report the first detection of galactic spiral structure by means of thermal emission from magnetically aligned dust grains. Our 89 $\mu$m polarimetric imaging of NGC 1068 with the High-resolution Airborne Wideband Camera/Polarimeter (HAWC+) on NAS
Externí odkaz:
http://arxiv.org/abs/1907.06648
Autor:
Angerhausen, D., Dreyer, C., Placek, B., Csizmadia, Sz., Eigmueller, Ph., Godolt, M., Kitzmann, D., Mallonn, M., Becklin, E. E., Collins, P., Dunham, E. W., Grenfell, J. L., Hamilton, R. T., Kabath, P., Logsdon, S. E., Mandell, A., Mandushev, G., McElwain, M., McLean, I. S., Pfueller, E., Rauer, H., Savage, M., Shenoy, S., Vacca, W. D., Van Cleve, J. E., Wiedemann, M., Wolf, J.
Publikováno v:
A&A 608, A120 (2017)
The benchmark exoplanet GJ 1214b is one of the best studied transiting planets in the transition zone between rocky Earth-sized planets and gas or ice giants. This class of super-Earth/mini-Neptune planets is unknown in our Solar System, yet is one o
Externí odkaz:
http://arxiv.org/abs/1708.07033
Autor:
Audard, M., Stringfellow, G. S., Güdel, M., Skinner, S. L., Walter, F. M., Guinan, E. F., Hamilton, R. T., Briggs, K. R., Baldovin-Saavedra, C.
Abriged version for astroph: The young late-type star V1118 Orionis was in outburst from 2005 to 2006. We followed the outburst with optical and near-infrared photometry; the X-ray emission was further probed with observations taken with XMM-Newton a
Externí odkaz:
http://arxiv.org/abs/0912.3224
Autor:
Audard, M., Guedel, M., Skinner, S. L., Briggs, K. R., Walter, F. M., Stringfellow, G., Hamilton, R. T., Guinan, E. F.
Publikováno v:
Astrophys.J.635:L81-L84,2005
We present results from a multi-wavelength campaign to monitor the 2005 outburst of the low-mass young star V1118 Ori. Although our campaign covers the X-ray, optical, infrared, and radio regimes, we focus in this Letter on the properties of the X-ra
Externí odkaz:
http://arxiv.org/abs/astro-ph/0510859
Autor:
Hamilton, R. T., Sion, E. M.
Using newly determined parallaxes for dwarf novae, we have derived outburst accretion rates for VY Aqr, RU Peg and T Leo and for T Leo during quiescence. The two short-period dwarf novae, VY Aqr and T Leo, show good agreement with optically thick ste
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408335
Autor:
Hamilton, R. T., Shergill, G. S.
Publikováno v:
Managerial and Decision Economics, 1993 Jan 01. 14(1), 47-52.
Externí odkaz:
https://www.jstor.org/stable/2487705
Autor:
Beesley, M. E., Hamilton, R. T.
Publikováno v:
The Journal of Industrial Economics, 1984 Dec 01. 33(2), 217-231.
Externí odkaz:
https://www.jstor.org/stable/2098510
Autor:
Hamilton, R. T., Butler, J. A. V.
Publikováno v:
Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character, 1932 Nov 01. 138(835), 450-459.
Externí odkaz:
https://www.jstor.org/stable/95969
Publikováno v:
Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1934 Dec 01. 147(862), 418-433.
Externí odkaz:
https://www.jstor.org/stable/96300