1 Ocak 2019 Dergi makalesi Açık Erişim

Busarev, V. V.; Shcherbina, M. P.; Barabanov, S. I.; Irsmambetova, T. R.; Kokhirova, G. I.; Khamroev, U. Kh.; Khamitov, I. M.; Bikmaev, I. F.; Gumerov, R. I.; Irtuganov, E. N.; Mel'nikov, S. S.

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        "name": "Busarev, V. V."
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        "affiliation": "Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow, Russia", 
        "name": "Shcherbina, M. P."
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      {
        "affiliation": "Russian Acad Sci, Inst Astron INASAN, Moscow, Russia", 
        "name": "Barabanov, S. I."
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      {
        "affiliation": "Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow, Russia", 
        "name": "Irsmambetova, T. R."
      }, 
      {
        "affiliation": "Acad Sci Republ Tajikistan, Inst Astrophys, Dushanbe, Tajikistan", 
        "name": "Kokhirova, G. I."
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      {
        "affiliation": "Acad Sci Republ Tajikistan, Inst Astrophys, Dushanbe, Tajikistan", 
        "name": "Khamroev, U. Kh."
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      {
        "name": "Khamitov, I. M."
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      {
        "name": "Bikmaev, I. F."
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      {
        "name": "Gumerov, R. I."
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        "name": "Irtuganov, E. N."
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      {
        "name": "Mel'nikov, S. S."
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    "description": "This paper presents the results that confirm the sublimation activity at the perihelion of the primitive main-belt asteroids 779 Nina, 704 Interamnia, and 145 Adeona; this activity was first discovered in September 2012 (Busarev et al., 2015; Busarev et al., 2016). The new spectrophotometric and/or UBVRI photometric observations of Nina, Interamnia, and Adeona were carried out in 2016-2018 during a regular perihelion passage of these asteroids. Additionally, probable spectral signs of weak sublimation activity were discovered on another two primitive main-belt asteroids, 51 Nemausa and 65 Cybele. In this study, we discuss the conditions for the occurrence of a periodic and/or continuous sublimation process on main-belt asteroids with low-temperature mineralogy; in particular, the conditions that are associated with their formation close to the \"snow line\" or beyond. We also consider general evolution processes that are able sustain a sufficiently high concentration of water ice close to the surface of the bodies in question and, therefore, their continuous sublimation activity, or lead to the recurrence of extinct activity.", 
    "doi": "10.1134/S0038094619040014", 
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    "journal": {
      "issue": "4", 
      "pages": "261-277", 
      "title": "SOLAR SYSTEM RESEARCH", 
      "volume": "53"
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    "title": "Confirmation of the Sublimation Activity of the Primitive Main-Belt Asteroids 779 Nina, 704 Interamnia, and 145 Adeona, as well as its Probable Spectral Signs on 51 Nemausa and 65 Cybele"
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