Reduction of asteroidal appulses. First results in Bucharest

Bibcode
1996RoAJ....6..199V
Vaduvescu, Ovidiu
Bibliographical reference

Romanian Astronomical Journal (1210-5168), Vol. 6, No. 2, p. 199 - 203 (1996)

Advertised on:
0
1996
Number of authors
1
IAC number of authors
0
Citations
0
Refereed citations
0
Description
The method presented is applied to asteroidal approaches to catalogue stars and occultations, and derives the minimum separation at conjunction and the corresponding time of these ones. Three CCD observations, reported to the European Asteroidal Occultation Network, illustrate the method.
Type
Refereed
Astrometry

It may interest you

  • Refereed
    An ultra-short-period super-Earth with an extremely high density and an outer companion
    We present the discovery and characterization of a new multi-planetary system around the Sun-like star K2-360 (EPIC 201595106). K2-360 was first identified in K2 photometry as the host of an ultra-short-period (USP) planet candidate with a period of 0.88 d. We obtained follow-up transit photometry, confirming the star as the host of the signal
    Livingston, John H. et al.

    Advertised on:

    11
    2024
    Bibcode
    2024NatSR..1427219L
    Citations
    0
  • Refereed
    Long-term Study of the 2020 Magnetar-like Outburst of the Young Pulsar PSR J1846-0258 in Kes 75
    Magnetar-like activity has been observed in a large variety of neutron stars. PSR J1846‑0258 is a young 327 ms radio-quiet pulsar with a large rotational power (∼8 × 10 36 erg s ‑1), and resides at the center of the supernova remnant Kes 75. It is one of the rare examples of a high-magnetic-field pulsar showing characteristics both of magnetars and
    Sathyaprakash, R. et al.

    Advertised on:

    11
    2024
    Bibcode
    2024ApJ...976...56S
    Citations
    0
  • Refereed
    Constraining the overcontact phase in massive binary evolution: III. Period stability of known B+B and O+B overcontact systems
    Context. Binary systems play a crucial role in massive star evolution. Systems composed of B-type and O-type stars are of particular interest due to their potential to lead to very energetic phenomena or the merging of exotic compact objects. Aims. We aim to determine the orbital period variations of a sample of B+B and O+B massive overcontact
    Vrancken, Jasmine et al.

    Advertised on:

    11
    2024
    Bibcode
    2024A&A...691A.150V
    Citations
    0