Zobrazeno 1 - 10
of 1 791
pro vyhledávání: '"Bolin B"'
Autor:
Bolin, B. T., Masci, F. J., Coughlin, M. W., Duev, D. A., Ivezić, Ž., Jones, R. L., Yoachim, P., Ahumada, T., Bhalerao, V., Choudhary, H., Contreras, C., Cheng, Y. -C., Copperwheat, C. M., Deshmukh, K., Fremling, C., Granvik, M., Hardegree-Ullman, K. K., Ho, A. Y. Q., Jedicke, R., Kasliwal, M., Kumar, H., Lin, Z. -Y., Mahabal, A., Monson, A., Neill, J. D., Nesvorný, D., Perley, D. A., Purdum, J. N., Quimby, R., Serabyn, E., Sharma, K., Swain, V.
Near-sun sky twilight observations allow for the detection of asteroid interior to the orbit of Venus (Aylos), the Earth (Atiras), and comets. We present the results of observations with the Palomar 48-inch telescope (P48)/Zwicky Transient Facility (
Externí odkaz:
http://arxiv.org/abs/2409.15263
Autor:
Athanasopoulos, D., Hanuš, J., Avdellidou, C., van Belle, G., Ferrero, A., Bonamico, R., Gazeas, K., Delbo, M., Rivet, J. P., Apostolovska, G., Todorović, N., Novakovic, B., Bebekovska, E. V., Romanyuk, Y., Bolin, B. T., Zhou, W., Agrusa, H.
Publikováno v:
A&A 690, A215 (2024)
The aim of our study is to characterise the spin states of the members of the Athor and Zita collisional families and test whether these members have a spin distribution consistent with a common origin from the break up of their respective family par
Externí odkaz:
http://arxiv.org/abs/2409.03419
The rotational properties of $\sim$10~m-scale asteroids are poorly understood with only a few measurements. Additionally, collisions or thermal recoil can spin their rotations to periods less than a few seconds obfuscating their study due to the obse
Externí odkaz:
http://arxiv.org/abs/2310.09290
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
Recently, the inner main belt asteroid (152830) Dinkinesh was identified as an additional fly-by target for the Lucy mission. The heliocentric orbit and approximate absolute magnitude of Dinkinesh are known, but little additional information was avai
Externí odkaz:
http://arxiv.org/abs/2303.08130
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
Autor:
Cooke, J., Angus, C., Auchettl, K., Bally, J., Bolin, B., Brough, S., Burchett, J. N., Foley, R., Foran, G., Forbes, D., Gannon, J., Hirai, R., Kacprzak, G. G., Margutti, R., Martinez-Lombilla, C., Mestric, U., Moller, A., Rest, A., Rhodes, J., Rich, R. M., Schussler, F., Wainscoat, R., Walawender, J., Wold, I., Zhang, J.
The Keck Wide-Field Imager (KWFI) is a proposed 1-degree diameter field of view UV-sensitive optical camera for Keck prime focus. KWFI will be the most powerful optical wide-field camera in the world and the only such 8m-class camera sensitive down t
Externí odkaz:
http://arxiv.org/abs/2207.11698
Autor:
Bolin, B. T., Ahumada, T., van Dokkum, P., Fremling, C., Hardegree-Ullman, K. K., Purdum, J. N., Serabyn, E., Southworth, J.
Near-Earth asteroids (NEAs) are organized into five main classes: Amor, Apollo, Aten, Atira and 'Ayl\'{o}'chaxnim. Asteroids belonging to the 'Ayl\'{o}'chaxnim class are located entirely within the orbit of Venus making them difficult to detect by gr
Externí odkaz:
http://arxiv.org/abs/2009.04125
Autor:
Regnier, Sean D., Stoops, William W., Lile, Joshua A., Alcorn, Joseph L., III, Bolin, B. Levi, Reynolds, Anna R., Hays, Lon R., Rayapati, Abner O., Rush, Craig R.
Publikováno v:
In Pharmacology, Biochemistry and Behavior March 2023 224
Autor:
Hanuš, J., Delbo', M., Alí-Lagoa, V., Bolin, B., Jedicke, R., Ďurech, J., Cibulková, H., Pravec, P., Kušnirák, P., Behrend, R., Marchis, F., Antonini, P., Arnold, L., Audejean, M., Bachschmidt, M., Bernasconi, L., Brunetto, L., Casulli, S., Dymock, R., Esseiva, N., Esteban, M., Gerteis, O., de Groot, H., Gully, H., Hamanowa, H., Krafft, P., Lehký, M., Manzini, F., Michelet, J., Morelle, E., Oey, J., Pilcher, F., Reignier, F., Roy, R., Salom, P. A., Warner, B. D.
Eos family was created during a catastrophic impact about 1.3 Gyr ago. Rotation states of individual family members contain information about the history of the whole population. We aim to increase the number of asteroid shape models and rotation sta
Externí odkaz:
http://arxiv.org/abs/1707.05507