Zobrazeno 1 - 10
of 76
pro vyhledávání: '"E. Bowell"'
Autor:
D. A. Oszkiewicz, K. Muinonen, E. Bowell, D. Trilling, L. H. Wasserman, A. Penttila, T. Pieniluoma
Publikováno v:
Atti della Accademia Peloritana dei Pericolanti : Classe di Scienze Fisiche, Matematiche e Naturali, Vol 89, Iss S1, Pp C1V89S1P072-1 (2011)
We present results obtained from processing large photometric data base. We make use of low-precision (generally rounded to 0.1 mag) and low-accuracy (rms magnitude uncertainties of ±0.2 to 0.3 mag) data obtained from the Minor Planet Center and mod
Externí odkaz:
https://doaj.org/article/b8daa050c3814a2f9bd97cf707a85e4e
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
E. Bowell, G.B. Valsecchi, K. Aksnes, J.-E. Arlot, A. Carusi, J.A. Fernández, A. Lemaître, B.G. Marsden, H. Rickman, V.A. Shor, D.K. Yeomans, J.-X. Zhang
Publikováno v:
Transactions of the International Astronomical Union. 25:187-198
Autor:
Mikhail Ya. Marov, G.M.F. A’Hearn, J. Baggaley, E. Bowell, S. Bowyer, D. Cruikshank, C. de Bergh, H. Keller, P. Lamy, V. Porubcan, J. Watanabe, I. Williams, V. Zappala
Publikováno v:
Transactions of the International Astronomical Union. 24:113-156
Autor:
Rita Schulz, K. Aksnes, J. Blue, E. Bowell, G. A. Burba, G. Consolmagno, R. Courtin, R. Lopes, M. Ya. Marov, B. G. Marsden, M. S. Robinson, V. V. Shevchenko, B. A. Smith
Publikováno v:
Transactions of the International Astronomical Union, Series B
XXVIIth IAU General Assembly
XXVIIth IAU General Assembly, Aug 2009, Rio de Janeiro, Brazil. pp.186-187, ⟨10.1017/S1743921310005016⟩
XXVIIth IAU General Assembly
XXVIIth IAU General Assembly, Aug 2009, Rio de Janeiro, Brazil. pp.186-187, ⟨10.1017/S1743921310005016⟩
The meeting was attended by 5 members of the WG (E. Bowell, G. Consolmagno, R. Courtain, R. Lopez, R. Schulz) one Task Group member (J. Watanabe), and several guests from the CSBN and CBAT. It was decided at the beginning of the meeting that the atte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::10184a382e265e41807b5f2cf8c49c16
https://hal.science/hal-03809707
https://hal.science/hal-03809707
Publikováno v:
Highlights of Astronomy. 12:255-256
We consider initial determination of orbits for trans-neptunian objects (TNOs), a topical theme because of the rapidly growing TNO population and the challenges in recovering lost TNOs. We apply the method of initial phase-space ranging of orbits to
Autor:
D. W. Dunham, J. B. Dunham, R. P. Binzel, D. S. Evans, M. Freuh, G. W. Henry, M. F. A'Hearn, R. G. Schnurr, R. Betts, H. Haynes, R. Orcutt, E. Bowell, L. H. Wasserman, R. A. Nye, H. L. Giclas, C. R. Chapman, R. D. Dietz, C. Moncivais, W. T. Douglass, D. C. Parker, J. D. Beish, J. O. Martin, D. R. Monger, W. B. Hubbard, H. J. Reitsema, A. R. Klemola, P. D. Lee, B. R. McNamara, P. D. Maley, P. Manly, N. L. Markworth, R. Nolthenius, T. D. Oswalt, J. A. Smith, E. F. Strother, H. R. Povenmire, R. D. Purrington, C. Trenary, G. H. Schneider, W. J. Schuster, M. A. Moreno, J. Guichard, G. R. Sanchez, G. E. Taylor, A. R. Upgren, T. C. von Flandern
Publikováno v:
The Astronomical Journal. 99:1636
The analysis and results of an occultation of the spectroscopic binary star 1 Vulpeculae by the asteroid (2) Pallas, observed from 130 locations, are presented. Combination of solutions from this and previous occultations shows the triaxial shape of
Publikováno v:
Icarus. 26:53-72
Isophotes of the luminance distribution over the disk of Venus at several phase angles and in several wavelengths are constructed by means of isodensitometry of high-quality photographic negatives of Venus. Twenty-three plates were selected from more
Autor:
L. Wasserman, E. Bowell
Publikováno v:
Symposium - International Astronomical Union. 109:231-236
The Lowell Observatory PDS is currently used in several projects which necessitate astrometric reduction of photographic plates. To meet this need, we have developed a series of computer programs for astrometric data reduction which enable the user t
Autor:
E. Bowell, B. Zellner
Publikováno v:
International Astronomical Union Colloquium. 39:185-197
A sample of 359 minor planets with available colorimetric, spectropnotometric, thermal-radiometric, and/or polarimetrie data are classified into broadly defined compositional types C (carbonaceous), S (silicaceous), M (metal-rich), E (metal-free; ens