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Results 1 - 18 of 18

Does the i-process operate at nearly solar metallicity?. (arXiv:2305.04189v1 [astro-ph.SR])
- Virtual Journal - Volume 21, 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])
- Virtual Journal - Volume 18, Issue 44 - article #5
- 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
- Virtual Journal - Volume 17, Issue 26 - article #8
- 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
S stars and s-process in the Gaia era I. Stellar parameters and chemical abundances in a sub-sample of S stars with new MARCS model atmospheres. (arXiv:1810.07105v1 [astro-ph.SR])
- Virtual Journal - Volume 16, Issue 42 - article #4
- Shreeya Shetye, Sophie Van Eck, Alain Jorissen, Hans Van Winckel, Lionel Siess, Stephane Goriely, Ana Escorza, Drisya Karinkuzhi, Bertrand Plez
- http://arxiv.org/abs/1810.07105
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])
- Virtual Journal - Volume 16, Issue 29 - article #20
- 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
Chemical analysis of three barium stars: HD 51959, HD 88035, HD 121447. (arXiv:1802.01343v1 [astro-ph.SR])
- Virtual Journal - Volume 16, Issue 6 - article #4
- Drisya Karinkuzhi (1), Aruna Goswami (1), Navin Sridhar (2), Thomas Masseron (3), Meenakshi Purandardas (1). ((1). Indian Institute of Astrophysics, Koramangala, Bangalore 560034, India. (2).Indian Institute of Science Education, Research, Bhopal Bhauri, Bhopal 462066, MP, India. (3). Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK)
- http://arxiv.org/abs/1802.01343
Chemical Analysis of a Carbon-enhanced Very Metal-poor Star: CD-27 14351
- Virtual Journal - Volume 15, Issue 1 - article #26
- Drisya Karinkuzhi, Aruna Goswami,, Thomas Masseron
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/834/1/61
Constraints of the Physics of Low-mass AGB Stars from CH and CEMP Stars
- Virtual Journal - Volume 14, Issue 52 - article #33
- S. Cristallo, D. Karinkuzhi, A. Goswami, L. Piersanti,, D. Gobrecht
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/833/2/181
Chemical analysis of a carbon-enhanced very metal-poor star: CD-27 14351. (arXiv:1611.01637v1 [astro-ph.SR])
- Virtual Journal - Volume 14, Issue 46 - article #4
- Drisya Karinkuzhi (1), Aruna Goswami (1), Thomas Masseron (2) ((1) Indian Institute of Astrophysics, Koramangala, Bangalore 560034, (2) Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK)
- http://arxiv.org/abs/1611.01637
Constraints of the physics of low-mass AGB stars from CH and CEMP stars. (arXiv:1610.05475v1 [astro-ph.SR])
- Virtual Journal - Volume 14, Issue 43 - article #7
- S. Cristallo, D. Karinkuzhi, A. Goswami, L. Piersanti, D. Gobrecht
- http://arxiv.org/abs/1610.05475
Abundance analysis of s-process enhanced barium stars
- Virtual Journal - Volume 14, Issue 39 - article #22
- Mahanta, U., Karinkuzhi, D., Goswami, A., Duorah, K.
- >Oxford University Press
- http://mnras.oxfordjournals.org/cgi/content/short/463/2/1213?rss=1
Abundance analysis of s-process enhanced barium stars. (arXiv:1608.06734v1 [astro-ph.SR])
- Virtual Journal - Volume 14, Issue 35 - article #2
- Upakul Mahanta (1,2), Drisya Karinkuzhi (3), Aruna Goswami (3), Kalpana Duorah (2) ((1). Department of Physics, Bajali College, Pathsala, Assam, 781325, India, (2). Department of Physics, Gauhati University, Guwahati 781014, Assam, India, (3). Indian Institute of Astrophysics, Koramangala, Bangalore 560034, India)
- http://arxiv.org/abs/1608.06734
Chemical analysis of CH stars - II: atmospheric parameters and elemental abundances
- Virtual Journal - Volume 12, Issue 25 - article #4
- Drisya Karinkuzhi (1,2), Aruna Goswami (1) ((1) Indian Institute of Astrophysics, Koramangala (2) Department of physics, Bangalore university)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 12 Dec
- arXiv:1412.3548 [pdf, ps, other]
Chemical analysis of CH stars - I: atmospheric parameters and elemental abundances
- Virtual Journal - Volume 12, Issue 23 - article #45
- Drisya Karinkuzhi (1,2), Aruna Goswami (1) ((1) Indian Institute of Astrophysics, Koramangala, India (2) Department of physics, Bangalore university, Jnana Bharathi Campus, Karnataka, India)
- arXiv.org - Astrophysics - Volume: 2014, Issue: 3 Oct
- arXiv:1410.0111 [pdf, ps, other]
HE 1015-2050: Discovery of a Hydrogen-deficient carbon star at high galactic latitude
- Virtual Journal - Volume 8, Issue 44 - article #8
- Aruna Goswami, Drisya Karinkuzhi, N. S. Shantikumar (1) ((1) Indian Institute of Astrophysics, Bangalore.)
- arXiv.org - Astrophysics - Volume: 2010, Issue: 29 Oct
- arXiv:1010.5094 [pdf, ps, other]
HE 1015–2050: Discovery of a Hydrogen-deficient Carbon Star at High Galactic Latitude
- Virtual Journal - Volume 8, Issue 43 - article #38
- Aruna Goswami, Drisya Karinkuzhi and N. S. Shantikumar
- The Astrophysical Journal Letters - Volume: 723, Issue: 2
- Abstract References Full text PDF (380 KB) View as HTML
The CH fraction of carbon stars at high Galactic latitudes
- Virtual Journal - Volume 8, Issue 20 - article #42
- Aruna Goswami, Drisya Karinkuzhi, N. S. Shantikumar
- Monthly Notices of the Royal Astronomical Society - Volume: 402, Issue: 2
- Abstract | References | Full Text: HTML, PDF (Size: 956K)
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The CH fraction of Carbon stars at high Galactic latitudes
- Virtual Journal - Volume 7, Issue 52 - article #9
- Aruna Goswami, Drisya Karinkuzhi, N. S. Shantikumar (Indian Institute of Astrophysics)
- arXiv.org - Astrophysics - Volume: 2009, Issue: 25 Dec
- arXiv:0912.4347 [ps, pdf, other]

Results 1 - 18 of 18

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