Projects funded by the NCN


Information on the principal investigator and host institution

Information of the project and the call

Keywords

Equipment

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The study of Accreting White Dwarf Binary Systems in Globular Clusters via Numerical Simulations

2016/21/N/ST9/02938

Keywords:

cataclysmic variables AM CVn symbiotic stars globular clusters stellar dynamics numerical simulations

Descriptors:

  • ST9_7: Stars and stellar systems

Panel:

ST9 - Astronomy and space science: astrophysics, astrochemistry, astrobiology, solar system, planetary systems, stellar, galactic and extragalactic astronomy, space science, instrumentation

Host institution :

Centrum Astronomiczne im. Mikołaja Kopernika Polskiej Akademii Nauk

woj. mazowieckie

Other projects carried out by the institution 

Principal investigator (from the host institution):

Diogo Belloni 

Number of co-investigators in the project: 2

Call: PRELUDIUM 11 - announced on 2016-03-15

Amount awarded: 72 200 PLN

Project start date (Y-m-d): 2017-03-15

Project end date (Y-m-d): 2018-03-30

Project duration:: 12 months (the same as in the proposal)

Project status: Project settled

Project description

Download the project description in a pdf file

Note - project descriptions were prepared by the authors of the applications themselves and placed in the system in an unchanged form.

Equipment purchased [PL]

  1. Pamięć masowa typu Lustre - 10 TB (1 416 PLN)
  2. Laptop (1 263 PLN)

Information in the final report

  • Publication in academic press/journals (5)
  1. Dynamical equivalence, the origin of the Galactic field stellar and binary population, and the initial radius-mass relation of embedded clusters
    Authors:
    Belloni, Diogo; Kroupa, Pavel; Rocha-Pinto, Helio J.; Giersz, Mirek
    Academic press:
    Monthly Notices of the Royal Astronomical Society (rok: 2018, tom: 474, strony: 3740-3745), Wydawca: Oxford University Press on behalf of the Royal Astronomical Society
    Status:
    Published
    DOI:
    10.1093/mnras/stx3034 - link to the publication
  2. MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- IV. cataclysmic variables -- properties of bright and faint populations
    Authors:
    Diogo Belloni; Mirek Giersz; Liliana E. Rivera-Sandoval
    Academic press:
    Monthly Notices of the Royal Astronomical Society (rok: 2018, ), Wydawca: Oxford University Press on behalf of the Royal Astronomical Society
    Status:
    Submitted
  3. MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters - III. Cataclysmic variables - implications of model assumptions
    Authors:
    Belloni, Diogo; Zorotovic, Mónica; Schreiber, Matthias R.; Leigh, Nathan W. C.; Giersz, Mirek; Askar, Abbas
    Academic press:
    Monthly Notices of the Royal Astronomical Society (rok: 2017, tom: 468, strony: 2429-2446), Wydawca: Oxford University Press on behalf of the Royal Astronomical Society
    Status:
    Published
    DOI:
    10.1093/mnras/stx575 - link to the publication
  4. On the initial binary population for star cluster simulations
    Authors:
    Belloni, Diogo; Askar, Abbas; Giersz, Mirek; Kroupa, Pavel; Rocha-Pinto, Helio J.
    Academic press:
    Monthly Notices of the Royal Astronomical Society (rok: 2017, tom: 471, strony: 2812-2828), Wydawca: Oxford University Press on behalf of the Royal Astronomical Society
    Status:
    Published
    DOI:
    10.1093/mnras/stx1763 - link to the publication
  5. No cataclysmic variables missing: higher merger rate brings into agreement observed and predicted space densities
    Authors:
    Diogo Belloni; Matthias R. Schreiber; Mónica Zorotovic; Krystian Iłkiewicz; Jarrod R. Hurley; Mirek Giersz; Felipe Lagos
    Academic press:
    Monthly Notices of the Royal Astronomical Society (rok: 2018, ), Wydawca: Oxford University Press on behalf of the Royal Astronomical Society
    Status:
    Submitted