Search Results - Sun's radius

Stress control of porous silicon films for microelectromechanical systems by Sun, Xiao, Keating, Adrian, Parish, Giacinta

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A study on the evolution of the contact angle of small punch creep test of Ductile materials by Cacciapuoti, B., Sun, Wei, McCartney, D.G.

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The roles of contact conformity, temperature and displacement amplitude on the lubricated fretting wear of a steel-on-steel contact by Warmuth, A.R., Sun, W., Shipway, P.H.

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Fretting wear mapping: the influence of contact geometry and frequency on debris formation and ejection for a steel-on-steel pair by Warmuth, A.R., Shipway, P.H., Sun, W.

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The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole by Leloudas, G., Fraser, M., Stone, N., van Velzen, S., Jonker, P., Arcavi, I., Fremling, C., Maund, J., Smartt, S., Krihler, T., Miller-Jones, James, Vreeswijk, P., Gal-Yam, A., Mazzali, P., De Cia, A., Howell, D., Inserra, C., Patat, F., Postigo, A., Yaron, O., Ashall, C., Bar, I., Campbell, H., Chen, T., Childress, M., Elias-Rosa, N., Harmanen, J., Hosseinzadeh, G., Johansson, J., Kangas, T., Kankare, E., Kim, S., Kuncarayakti, H., Lyman, J., Magee, M., Maguire, K., Malesani, D., Mattila, S., McCully, C., Nicholl, M., Prentice, S., Romero-Canizales, C., Schulze, S., Smith, K., Sollerman, J., Sullivan, M., Tucker, B., Valenti, S., Wheeler, J., Young, D.

“…For a star with the mass of the Sun (M ⊙) and a non-spinning black hole with a mass <10 8 M ⊙, the tidal radius lies outside the black hole event horizon2 and the disruption results in a luminous flare. …”
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Two stellar-mass black holes in the globular cluster M22 by Strader, J., Chomiuk, L., Maccarone, T., Miller-Jones, James, Seth, A.

“…The identification of two black holes in one cluster shows that ejection of black holes is not as efficient as predicted by most models, and we argue that M22 may contain a total population of ~5–100 black holes. The large core radius of M22 could arise from heating produced by the black holes.…”
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Attitude Determination And Control For Stabilization And Pointing Accuracy For 3u Class Nano-Satellite by Fadly, Muhammad

“…The controller is able to maintain the stability only in small radius position from its design point but if the satellite go beyond the radius the new controller must be recalculated. …”
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MOA-2007-BLG-197: Exploring the brown dwarf desert by Ranc, C., Cassan, A., Albrow, M., Kubas, D., Bond, I., Batista, V., Beaulieu, J., Bennett, D., Dominik, M., Dong, S., Fouqué, P., Gould, A., Greenhill, J., Jørgensen, U., Kains, N., Menzies, J., Sumi, T., Bachelet, E., Coutures, C., Dieters, S., Dominis Prester, D., Donatowicz, J., Gaudi, B., Han, C., Hundertmark, M., Horne, K., Kane, S., Lee, C., Marquette, J., Park, B., Pollard, K., Sahu, K., Street, R., Tsapras, Y., Wambsganss, J., Williams, Andrew, Zub, M., Abe, F., Fukui, A., Itow, Y., Masuda, K., Matsubara, Y., Muraki, Y., Ohnishi, K., Rattenbury, N., Saito, T., Sullivan, D., Sweatman, W., Tristram, P., Yock, P., Yonehara, A.

“…We present the analysis of MOA-2007-BLG-197Lb, the first brown dwarf companion to a Sun-like star detected through gravitational microlensing. …”
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The effect of the galaxy environment on the size and structure of galaxies by Maltby, David Terence

“…For elliptical, lenticular, and high-mass (M* > 10^10 M_sun) spirals, we find no evidence to suggest that a galaxy's size (i.e. effective radius a_e) is dependent on the environment. …”
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