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Does the i-process operate at nearly solar metallicity?. (arXiv:2305.04189v1 [astro-ph.SR])
- Volume 18, Issue 19 - article #3
- D. Karinkuzhi (1,2), S. Van Eck (2), S. Goriely (2), L. Siess (2), A. Jorissen (2), A. Choplin (2), A. Escorza (3), S. Shetye (4), H. Van Winckel (5). ((1). Department of Physics, University of Calicut, Thenhipalam, Malappuram 673635, India (2). Institut d'Astronomie et d'Astrophysique, Universit'e Libre de Bruxelles (ULB) C.P. 226, B-1050 Bruxelles, Belgium (3). European Southern Observatory, Alonso de Córdova 3107, Vitacura, Casilla 19001, Santiago de Chile, Chile (4). Institute of Physics, Laboratory of Astrophysics, École polytechnique fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland (5).Instituut voor Sterrenkunde, KULeuven, Celestijnenlaan 200D, 3001 Leuven, Belgium)
- http://arxiv.org/abs/2305.04189
Low-mass low-metallicity AGB stars as an efficient i-process site explaining CEMP-rs stars. (arXiv:2010.13620v1 [astro-ph.SR])
- Volume 15, Issue 44 - article #6
- D. Karinkuzhi (1,2,3), S. Van Eck (2), S. Goriely (2), L. Siess (2), A. Jorissen (2), T. Merle (2), A. Escorza (2,4), T. Masseron (5,6) ((1). Department of Physics, Indian Institute of Science, Bangalore, India.560012, (2). Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, ULB, Campus Plaine C.P. 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium, (3). Department of Physics, Jnana Bharathi Campus, Bangalore University, Bangalore, India. 560056, (4). Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium, (5). Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain, (6). Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain)
- http://arxiv.org/abs/2010.13620
Barium and related stars, and their white-dwarf companions
- Volume 14, Issue 26 - article #9
- A. Jorissen, H. M. J. Boffin, D. Karinkuzhi, S. Van Eck, A. Escorza, S. Shetye, H. Van Winckel
- Astronomy & Astrophysics
- http://feedproxy.google.com/~r/edp_aa/~3/M3fJl4TJmrA/201834630
Barium & related stars and their white-dwarf companions I. Giant stars. (arXiv:1904.03975v1 [astro-ph.SR])
- Volume 14, Issue 15 - article #2
- A. Jorissen, H.M.J. Boffin, D. Karinkuzhi, S. Van Eck, A. Escorza, S. Shetye, H. Van Winckel
- http://arxiv.org/abs/1904.03975
Barium & related stars and their white-dwarf companions II. Main-sequence and subgiant stars. (arXiv:1904.04095v1 [astro-ph.SR])
- Volume 14, Issue 15 - article #3
- A. Escorza, D. Karinkuzhi, A. Jorissen, L. Siess, H. Van Winckel, D. Pourbaix, C. Johnston, B. Miszalski, G-M. Oomen, M. Abdul-Masih, H.M.J. Boffin, P. North, R. Manick, S. Shetye, J. Mikołajewska
- http://arxiv.org/abs/1904.04095
When binaries keep track of recent nucleosynthesis: The Zr - Nb pair in extrinsic stars as an s-process diagnostic. (arXiv:1807.06332v1 [astro-ph.SR])
- Volume 13, Issue 29 - article #16
- D. Karinkuzhi (1), S. Van Eck (1), A. Jorissen (1), S. Goriely (1), L. Siess (1), T. Merle (1), A. Escorza (1, 2), M. Van der Swaelmen (1), H.M.J. Boffin (3), T. Masseron (4,5), S. Shetye (1,2), B. Plez (6) ((1). Institute of Astronomy, Astrophysics, University of Brussels, ULB, Campus Plaine C.P. 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium. (2) Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium. (3) ESO, Karl Schwarzschild Strasse 2, D-85748 Garching bei Munchen, Germany. (4) Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain. (5) Departamento de Astrofisica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain. (6) Laboratoire Univers et Particules de Montpellier, Universite Montpellier, CNRS, 34095, Montpellier Cedex 05, France.)
- http://arxiv.org/abs/1807.06332
Constraints of the Physics of Low-mass AGB Stars from CH and CEMP Stars
- Volume 11, Issue 52 - article #12
- S. Cristallo, D. Karinkuzhi, A. Goswami, L. Piersanti,, D. Gobrecht
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/833/2/181

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