Zobrazeno 1 - 10
of 157
pro vyhledávání: '"Mutchler, M."'
The $\sim$4 km diameter main belt asteroid 6478 Gault has ejected dust intermittently since at least 2013. The character of the emission, including its episodic nature and the low speed of the ejected particles ($V \sim $ 0.15 m s$^{-1}$), is most co
Externí odkaz:
http://arxiv.org/abs/2103.05601
Autor:
Moreno, F., Licandro, J., Mutchler, M., Cabrera-Lavers, A., Pinilla-Alonso, N., Pozuelos, F. J.
After the early observations of the disrupted asteroid P/2016 G1 with the 10.4m Gran Telescopio Canarias (GTC), and the modeling of the dust ejecta, we have performed a follow-up observational campaign of this object using the Hubble Space Telescope
Externí odkaz:
http://arxiv.org/abs/1711.01793
Autor:
Stern, S. A., Bagenal, F., Ennico, K., Gladstone, G. R., Grundy, W. M., McKinnon, W. B., Moore, J. M., Olkin, C. B., Spencer, J. R., Weaver, H. A., Young, L. A., Andert, T., Andrews, J., Banks, M., Bauer, B., Bauman, J., Barnouin, O. S., Bedini, P., Beisser, K., Beyer, R. A., Bhaskaran, S., Binzel, R. P., Birath, E., Bird, M., Bogan, D. J., Bowman, A., Bray, V. J., Brozovic, M., Bryan, C., Buckley, M. R., Buie, M. W., Buratti, B. J., Bushman, S. S., Calloway, A., Carcich, B., Cheng, A. F., Conard, S., Conrad, C. A., Cook, J. C., Cruikshank, D. P., Custodio, O. S., Ore, C. M. Dalle, Deboy, C., Dischner, Z. J. B., Dumont, P., Earle, A. M., Elliott, H. A., Ercol, J., Ernst, C. M., Finley, T., Flanigan, S. H., Fountain, G., Freeze, M. J., Greathouse, T., Green, J. L., Guo, Y., Hahn, M., Hamilton, D. P., Hamilton, S. A., Hanley, J., Harch, A., Hart, H. M., Hersman, C. B., Hill, A., Hill, M. E., Hinson, D. P., Holdridge, M. E., Horanyi, M., Howard, A. D., Howett, C. J. A., Jackman, C., Jacobson, R. A., Jennings, D. E., Kammer, J. A., Kang, H. K., Kaufmann, D. E., Kollmann, P., Krimigis, S. M., Kusnierkiewicz, D., Lauer, T. R., Lee, J. E., Lindstrom, K. L., Linscott, I. R., Lisse, C. M., Lunsford, A. W., Mallder, V. A., Martin, N., McComas, D. J., McNutt Jr., R. L., Mehoke, D., Mehoke, T., Melin, E. D., Mutchler, M., Nelson, D., Nimmo, F., Nunez, J. I., Ocampo, A., Owen, W. M., Paetzold, M., Page, B., Parker, A. H., Parker, J. W., Pelletier, F., Peterson, J., Pinkine, N., Piquette, M., Porter, S. B., Protopapa, S., Redfern, J., Reitsema, H. J., Reuter, D. C., Roberts, J. H., Robbins, S. J., Rogers, G., Rose, D., Runyon, K., Retherford, K. D., Ryschkewitsch, M. G., Schenk, P., Schindhelm, R., Sepan, B., Showalter, M. R., Singer, K. N., Soluri, M., Stanbridge, D., Steffl, A. J., Strobel, D. F., Stryk, T., Summers, M. E., Szalay, J. R., Tapley, M., Taylor, A., Taylor, H., Throop, H. B., Tsang, C. C. C., Tyler, G. L., Umurhan, O. M., Verbiscer, A. J., Versteeg, M. H., Vincent, M., Webbert, R., Weidner, S., Weigle II, G. E., White, O. L., Whittenburg, K., Williams, B. G., Williams, K., Williams, S., Woods, W. W., Zangari, A. M., Zirnstein, E.
Publikováno v:
Science, vol 350, 292, 2015
The Pluto system was recently explored by NASA's New Horizons spacecraft, making closest approach on 14 July 2015. Pluto's surface displays diverse landforms, terrain ages, albedos, colors, and composition gradients. Evidence is found for a water-ice
Externí odkaz:
http://arxiv.org/abs/1510.07704
Autor:
Ryan Jr., R. E., McCarthy, P. J., Cohen, S. H., Yan, H., Hathi, N. P., Koekemoer, A. M., Rutkowski, M. J., Mechtley, M. R., Windhorst, R. A., O'Connell, R. W., Balick, B., Bond, H. E., Bushouse, H., Calzetti, D., Crockett, R. M., Disney, M., Dopita, M. A., Frogel, J. A., Hall, D. N. B., Holtzman, J. A., Kaviraj, S., Kimble, R. A., MacKenty, J., Mutchler, M., Paresce, F., Saha, A., Silk, J. I., Trauger, J., Walker, A. R., Whitmore, B. C., Young, E.
We present results on the size evolution of passively evolving galaxies at 1
Externí odkaz:
http://arxiv.org/abs/1007.1460
Autor:
Straughn, A. N., Kuntschner, H., Kuemmel, M., Walsh, J. R., Cohen, S. H., Gardner, J. P., Windhorst, R. A., O'Connell, R. W., Pirzkal, N., Meurer, G., McCarthy, P. J., Hathi, N. P., Malhotra, S., Rhoads, J., Balick, B., Bond, H. E., Calzetti, D., Disney, M. J., Dopita, M. A., Frogel, J. A., Hall, D. N. B., Holtzman, J. A., Kimble, R. A., Mutchler, M., Luppino, G., Paresce, F., Saha, A., Silk, J. I., Trauger, J. T., Walker, A. R., Whitmore, B. C., Young, E. T., Xu, C.
We present grism spectra of emission-line galaxies (ELGs) from 0.6-1.6 microns from the Wide Field Camera 3 on the Hubble Space Telescope. These new infrared grism data augment previous optical Advanced Camera for Surveys G800L 0.6-0.95 micron grism
Externí odkaz:
http://arxiv.org/abs/1005.3071
Autor:
Weaver, H. A., Feldman, P. D., Merline, W. J., Mutchler, M. J., A'Hearn, M. F., Bertaux, J. -L., Feaga, L. M., Parker, J. W., Slater, D. C., Steffl, A. J., Chapman, C. R., Drummond, J. D., Stern, S. A.
The asteroid (21) Lutetia is the target of a planned close encounter by the Rosetta spacecraft in July 2010. To prepare for that flyby, Lutetia has been extensively observed by a variety of astronomical facilities. We used the Hubble Space Telescope
Externí odkaz:
http://arxiv.org/abs/0912.4572
Autor:
Mutchler, M., Bond, H. E., Christian, C. A., Frattare, L. M., Hamilton, F., Januszewski, W., Levay, Z. G., Mountain, M., Noll, K. S., Royle, P., Gallagher, J. S., Puxley, P.
In March 2006, the Hubble Heritage Team obtained a large four-filter (B, V, I, and H-alpha) six-point mosaic dataset of the prototypical starburst galaxy NGC 3034 (M82), with the Advanced Camera for Surveys (ACS) onboard the Hubble Space Telescope (H
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612547
Pluto's two small satellites, temporarily designated S/2005 P 1 and S/2005 P 2, were observed on four dates (15.1 and 18.1 May 2005, 15.7 February 2006, and 2.8 March 2006) using the Hubble Space Telescope's (HST) Advanced Camera for Surveys (ACS). H
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605014
Autor:
Weaver, H. A., Stern, S. A., Mutchler, M. J., Steffl, A. J., Buie, M. W., Merline, W. J., Spencer, J. R., Young, E. F., Young, L. A.
Pluto's first known moon, Charon, was discovered in 1978 (Christy 1978) and has a diameter about half that of Pluto (Buie 1992,Young 1994, Sicardy 2005), which makes it larger relative to its primary than any other moon in the Solar System. Previous
Externí odkaz:
http://arxiv.org/abs/astro-ph/0601018
Autor:
Stern, S. A., Weaver, H. A., Steffl, A. J., Mutchler, M. J., Merline, W. J., Buie, M. W., Young, E. F., Young, L. A., Spencer, J. R.
Our discovery of two new satellites of Pluto, designated S/2005 P 1 and S/2005 P 2 (henceforth, P1 and P2), combined with the constraints on the absence of more distant satellites of Pluto, reveal that Pluto and its moons comprise an unusual, highly
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512599