Pregled bibliografske jedinice broj: 998579
Revealing δ Cephei's Secret Companion and Intriguing Past
Revealing δ Cephei's Secret Companion and Intriguing Past // The Astrophysical journal, 804 (2015), 2; 144, 11 doi:10.1088/0004-637x/804/2/144 (međunarodna recenzija, članak, znanstveni)
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Naslov
Revealing δ Cephei's Secret Companion and Intriguing Past
Autori
Anderson, R. I. ; Sahlmann, J. ; Holl, B. ; Eyer, L. ; Palaversa, L. ; Mowlavi, N. ; Süveges, M. ; Roelens, M.
Izvornik
The Astrophysical journal (0004-637X) 804
(2015), 2;
144, 11
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
binaries: general ; binaries: spectroscopic ; stars: distances ; stars: individual: δ Cephei & HD 213306 & HIP 110991 ; stars: oscillations ; stars: variables: Cepheids
Sažetak
Classical Cepheid variable stars are crucial calibrators of the cosmic distance scale thanks to a relation between their pulsation periods and luminosities. Their archetype, δ Cephei, is an important calibrator for this relation. In this paper, we show that δ Cephei is a spectroscopic binary based on newly obtained high-precision radial velocities. We combine these new data with literature data to determine the orbit, which has period 2201 days, semi-amplitude 1.5 km s-1, and high eccentricity (e = 0.647). We re-analyze Hipparcos intermediate astrometric data to measure δ Cephei's parallax (\varpi =4.09+/- 0.16 mas) and find tentative evidence for an orbital signature, although we cannot claim detection. We estimate that Gaia will fully determine the astrometric orbit. Using the available information from spectroscopy, velocimetry, astrometry, and Geneva stellar evolution models ({; ; {; ; M}; ; δ Cep}; ; ˜ 5.0-5.25 {; ; {; ; M}; ; ⊙ }; ; ), we constrain the companion mass to within 0.2 {; ; {; ; M}; ; ⊙ }; ; \lt {; ; {; ; M}; ; 2}; ; \lt 1.2. We discuss the potential of ongoing and previous interactions between the companion and δ Cephei near pericenter passage, informing reported observations of circumstellar material and bow shock. The orbit may have undergone significant changes due to a Kozai-Lidov mechanism driven by the outer (visual and astrometric) companion HD 213307. Our discovery of δ Cephei's nature as a spectroscopic binary exposes a hidden companion and reveals a rich and dynamical history of the archetype of classical Cepheid variables.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
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