Zobrazeno 1 - 10
of 280
pro vyhledávání: '"Lisse, C. M."'
Stellar winds of cool main sequence stars are very difficult to constrain observationally. One way to measure stellar mass loss rates is to detect soft X-ray emission from stellar astrospheres produced by charge exchange between heavy ions of the ste
Externí odkaz:
http://arxiv.org/abs/2404.14980
Autor:
Bolin, B. T., Masci, F. J., Duev, D. A., Milburn, J. W., Purdum, J. N., Avdellidou, C., Cheng, Y. -C., Delbo, M., Fremling, C., Ghosal, M., Lin, Z. -Y., Lisse, C. M., Mahabal, A., Saki, M.
Long-period comets are planetesimal remnants constraining the environment and volatiles of the protoplanetary disc. We report the discovery of hyperbolic long-period comet C/2022 E3 (ZTF), which has a perihelion $\sim$1.11 au, an eccentricity $\gtrsi
Externí odkaz:
http://arxiv.org/abs/2309.14336
Autor:
Bolin, B. T., Fremling, C., Morbidelli, A., Noll, K. S., van Roestel, J., Deibert, E. K., Delbo, M., Gimeno, G., Heo, J. -E., Lisse, C. M., Seccull, T., Suh, H.
Neptunian Trojans (NTs), trans-Neptunian objects in 1:1 mean-motion resonance with Neptune, are generally thought to have been captured from the original trans-Neptunian protoplanetary disk into co-orbital resonance with the ice giant during its outw
Externí odkaz:
http://arxiv.org/abs/2302.04280
Publikováno v:
Icarus 2014, Volume 231, p. 338-355
We obtained mid-infrared spectra of chondrules, matrix, CAIs and bulk material from primitive type 1-4 chondrites in order to compare them with the dust material in young, forming solar systems and around comets. Our aim is to investigate whether the
Externí odkaz:
http://arxiv.org/abs/2212.14835
Publikováno v:
Icarus (2012), Volume 219, Issue 1, p. 48-56
Mid-infrared (5 micron to 25 micron) transmission/absorption spectra of differentiated meteorites (achondrites) were measured to permit comparison with astronomical observations of dust in different stages of evolution of young stellar objects. In co
Externí odkaz:
http://arxiv.org/abs/2212.13959
Publikováno v:
Icarus (2014), Volume 239, p. 1-14
In order to link infrared observations of dust formed during planet formation in debris disks to mid-infrared spectroscopic data of planetary materials from differentiated terrestrial and asteroidal bodies, we obtained absorption spectra of a represe
Externí odkaz:
http://arxiv.org/abs/2212.13174
Autor:
Lisse, C. M., Steckloff, J. K., Prialnik, D., Womack, M., Harrington-Pinto, O., Sarid, G., Fernandez, Y. R., Schambeau, C. A., Kareta, T., Samarasinha, N. H., Harris, W., Volk, K., Woodney, L. M., Cruikshank, D. P., Sandford, S. A.
Centaur 29P/Schwassmann-Wachmann 1 (SW1) is a highly active object orbiting in the transitional Gateway region (Sarid et al. 2019) between the Centaur and Jupiter Family Comet regions. SW1 is unique among the Centaurs in that it experiences quasi-reg
Externí odkaz:
http://arxiv.org/abs/2209.09136
Autor:
Lisse, C. M., Steckloff, J. K.
In 2010 Jewitt and Li published a paper examining the behavior of comet-asteroid transition object 3200 Phaethon, arguing it was asteroid-like in its behavior throughout most of its orbit, but that near its perihelion, at a distance of only 0.165 AU
Externí odkaz:
http://arxiv.org/abs/2203.09876
Autor:
Lisse, C. M., Gladstone, G. R., Young, L. A., Cruikshank, D. P., Sandford, S. A., Schmitt, B., Stern, S. A., Weaver, H. A., Umurhan, O., Pendleton, Y. J., Keane, J. T., Parker, J. M., Binzel, R. P., Earle, A. M., Horanyi, M., El-Maarry, M., Cheng, A. F., Moore, J. M., McKinnon, W. B., Grundy, W. M., Kavelaars, J. J., Linscott, I. R., Lyra, W., Lewis, B. L., Britt, D. T., Spencer, J. R., Olkin, C. B., McNutt, R. L., Elliott, H. A., Dello-Russo, N., Steckloff, J. K., Neveu, M., Mousis, O.
We present new, ice species-specific New Horizons/Alice upper gas coma production limits from the 01 Jan 2019 MU69/Arrokoth flyby of Gladstone et al. (2021) and use them to make predictions about the rarity of majority hypervolatile (CO, N$_2$, CH$_4
Externí odkaz:
http://arxiv.org/abs/2203.08888
Autor:
Umurhan, O. M., Grundy, W. M., Bird, M. K., Beyer, R., Keane, J. T., Linscott, I. R., Birch, S., Bierson, C., Young, L. A., Stern, S. A., Lisse, C. M., Howett, C. J. A., Protopapa, S., Spencer, J. R., Binzel, R. P., Mckinnon, W. B., Lauer, T. R., Weaver, H. A., Olkin, C. B., Singer, K. N., Verbiscer, A. J., Parker, A. H.
A near surface thermal model for Arrokoth is developed based on the recently released $10^5$ facet model of the body. This thermal solution takes into account Arrokoth's surface re-radiation back onto itself. The solution method exploits Arrokoth's p
Externí odkaz:
http://arxiv.org/abs/2202.10485