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Pregled bibliografske jedinice broj: 998579

Revealing δ Cephei's Secret Companion and Intriguing Past


Anderson, R. I.; Sahlmann, J.; Holl, B.; Eyer, L.; Palaversa, L.; Mowlavi, N.; Süveges, M.; Roelens, M.
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



POVEZANOST RADA


Profili:

Avatar Url Lovro Palaversa (autor)

Poveznice na cjeloviti tekst rada:

doi iopscience.iop.org

Citiraj ovu publikaciju:

Anderson, R. I.; Sahlmann, J.; Holl, B.; Eyer, L.; Palaversa, L.; Mowlavi, N.; Süveges, M.; Roelens, M.
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)
Anderson, R., Sahlmann, J., Holl, B., Eyer, L., Palaversa, L., Mowlavi, N., Süveges, M. & Roelens, M. (2015) Revealing δ Cephei's Secret Companion and Intriguing Past. The Astrophysical journal, 804 (2), 144, 11 doi:10.1088/0004-637x/804/2/144.
@article{article, author = {Anderson, R. I. and Sahlmann, J. and Holl, B. and Eyer, L. and Palaversa, L. and Mowlavi, N. and S\"{u}veges, M. and Roelens, M.}, year = {2015}, pages = {11}, DOI = {10.1088/0004-637x/804/2/144}, chapter = {144}, keywords = {binaries: general, binaries: spectroscopic, stars: distances, stars: individual: δ Cephei and HD 213306 and HIP 110991, stars: oscillations, stars: variables: Cepheids}, journal = {The Astrophysical journal}, doi = {10.1088/0004-637x/804/2/144}, volume = {804}, number = {2}, issn = {0004-637X}, title = {Revealing δ Cephei's Secret Companion and Intriguing Past}, keyword = {binaries: general, binaries: spectroscopic, stars: distances, stars: individual: δ Cephei and HD 213306 and HIP 110991, stars: oscillations, stars: variables: Cepheids}, chapternumber = {144} }
@article{article, author = {Anderson, R. I. and Sahlmann, J. and Holl, B. and Eyer, L. and Palaversa, L. and Mowlavi, N. and S\"{u}veges, M. and Roelens, M.}, year = {2015}, pages = {11}, DOI = {10.1088/0004-637x/804/2/144}, chapter = {144}, keywords = {binaries: general, binaries: spectroscopic, stars: distances, stars: individual: δ Cephei and HD 213306 and HIP 110991, stars: oscillations, stars: variables: Cepheids}, journal = {The Astrophysical journal}, doi = {10.1088/0004-637x/804/2/144}, volume = {804}, number = {2}, issn = {0004-637X}, title = {Revealing δ Cephei's Secret Companion and Intriguing Past}, keyword = {binaries: general, binaries: spectroscopic, stars: distances, stars: individual: δ Cephei and HD 213306 and HIP 110991, stars: oscillations, stars: variables: Cepheids}, chapternumber = {144} }

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


Citati:





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