258 citations
- Z. Eker2 profiles19 · h 18
- S. Bilir2 profiles11 · h 22
- F. Soydugan2 profiles10 · h 14
- B. C. Lütfüoğlu2 profiles9 · h 20
- F. Cappuzzello2 profiles9 · h 33
- H. Hassanabadi4 profiles9 · h 24
- D. Carbone2 profiles8 · h 29
- D. Torresi2 profiles8
- F. Delaunay3 profiles8 · h 22
- M. Cavallaro2 profiles8 · h 32
- O. Sgouros2 profiles8
- A. Foti7 · h 31
- Çanakkale Onsekiz Mart ÜniversitesiTR16 papers
- Istanbul UniversityTR16 papers
- TÜBİTAK National ObservatoryTR13 papers
- University of Hradec KrálovéCZ13 papers
- Centre National de la Recherche ScientifiqueFR10 papers
- University of ShahroodIR9 papers
- Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del SudIT8 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di TorinoIT8 papers
- Universidad Nacional Autónoma de MéxicoMX8 papers
- University of CataniaIT8 papers
- National and Kapodistrian University of AthensGR7 papers
- Universidade de São PauloBR7 papers
6 papers · 1 filter
Physical properties of the slow-rotating near-Earth asteroid (2059) Baboquivari from one apparition
Orhan Erece, Irek Khamitov, Murat Kaplan +6
In this study, we carried out photometric, spectroscopic, and for the first time, polarimetric observations of the Amor-type near-Earth asteroid (2059) Baboquivari. Our findings re…
The two rings of (50000) Quaoar
C. L. Pereira, B. Sicardy, B. E. Morgado +66
Quaoar is a classical Trans-Neptunian Object (TNO) with an area equivalent diameter of 1,100 km and an orbital semi-major axis of 43.3 astronomical units. Based on stellar occultat…
Refinement of the convex shape model and tumbling spin state of (99942) Apophis using the 2020-2021 apparition data
H. -J. Lee, M. -J. Kim, A. Marciniak +30
Context. The close approach of the near-Earth asteroid (99942) Apophis to Earth in 2029 will provide a unique opportunity to examine how the physical properties of the asteroid cou…
Horseshoe Co-orbitals of Earth: Current Population and New Candidates
Murat Kaplan, Sergen Cengiz
Most co-orbital objects in the Solar system are thought to follow tadpole-type orbits, behaving as Trojans. However, most of Earth's identified co-orbitals are moving along horsesh…
The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation
J. L. Ortiz, P. Santos-Sanz, B. Sicardy +90
Among the four known transneptunian dwarf planets, Haumea is an exotic, very elongated, and fast rotating body. In contrast to the other dwarf planets, its size, shape, albedo, and…
Shape and spin determination of Barbarian asteroids
M. Devogèle, P. Tanga, P. Bendjoya +51
Context. The so-called Barbarian asteroids share peculiar, but common polarimetric properties, probably related to both their shape and composition. They are named after (234) Barb…