Pregled bibliografske jedinice broj: 962672
Evidence for conservative mass transfer in the classical Algol system δ Librae from its surface carbon-to-nitrogen abundance ratio
Evidence for conservative mass transfer in the classical Algol system δ Librae from its surface carbon-to-nitrogen abundance ratio // Monthly notices of the Royal Astronomical Society, 481 (2018), 4; 5660-5674 doi:0.1093/mnras/sty2684 (međunarodna recenzija, članak, znanstveni)
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Naslov
Evidence for conservative mass transfer in the classical Algol system δ Librae from its surface carbon-to-nitrogen abundance ratio
Autori
Dervisoglu, A. ; Pavlovski, K. ; Lehmann, H., ; Southworth, J. ; Bewsher, D.
Izvornik
Monthly notices of the Royal Astronomical Society (0035-8711) 481
(2018), 4;
5660-5674
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
chemical abundances ; eclipsing binaries ; spectroscopic binaries ; stellar evolution
Sažetak
Algol-type binary systems are the product of rapid mass transfer between the initially more massive component to its companion. It is still unknown whether the process is conservative, or whether substantial mass is lost from the system. The history of a system prior to mass exchange is imprinted in the photospheric chemical composition, in particular in the carbon- to-nitrogen (C/N) ratio. We use this to trace the efficiency of mass-transfer processes in the components of a classical Algol-type system, δ Librae. The present analysis is based on new spectroscopic data (ground- based high-resolution e ́chelle spectra) and extracted archival photometric observations (space-based measurements from the STEREO satellites). In the orbital solution, non-Keplerian effects on the radial-velocity variations were taken into account. This reduces the primary’s mass by 1.1 M⊙ (∼23 per cent) significantly in comparison to previous studies, and removes a long-standing discrepancy between the radius and effective temperature. A spectral disentangling technique is applied to the e ́chelle observations and the spectra of the individual components are separated. Atmospheric and abundance analyses are performed for the mass-gaining component and we found C/N =1.55 ± 0.40 for this star. An extensive set of evolutionary models (3.5 × 10^6) for both components are calculated from which the best-fitting model is derived. It is found that β, the parameter that quantifies the efficiency of mass-loss from a binary system, is close to zero. This means that the mass transfer in δ Lib is mostly conservative with little mass-loss from the system.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
HRZZ-IP-2014-09-8656 - Zvijezde i prašina: struktura, sastav i interakcija (STARDUST) (Pavlovski, Krešimir, HRZZ - 2014-09) ( CroRIS)
Ustanove:
Prirodoslovno-matematički fakultet, Zagreb
Profili:
Krešimir Pavlovski
(autor)
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus