Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Alina G. Istrate"'
Autor:
Jianxing Chen, Mario Cadelano, Cristina Pallanca, Francesco R. Ferraro, Barbara Lanzoni, Alina G. Istrate, Marta Burgay, Paulo C. C. Freire, Tasha Gautam, Andrea Possenti, Alessandro Ridolfi
Publikováno v:
The Astrophysical Journal, Vol 948, Iss 2, p 84 (2023)
We report on the discovery of the companion star to the millisecond pulsar PSR J1835−3259B in the Galactic globular cluster NGC 6652. Taking advantage of deep photometric archival observations acquired through the Hubble Space Telescope in near-UV
Externí odkaz:
https://doaj.org/article/56f32c49008f4b7f83ea56f954e2ae82
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 494, 4031-4042
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 494, 3, pp. 4031-4042
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 494, 3, pp. 4031-4042
Binaries harbouring millisecond pulsars enable a unique path to determine neutron star masses: radio pulsations reveal the motion of the neutron star, while that of the companion can be characterised through studies in the optical range. PSR J1012+53
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 510, 1, pp. 858-869
Monthly Notices of the Royal Astronomical Society, 510, 858-869
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Monthly Notices of the Royal Astronomical Society, 510, 858-869
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Pulsating low-mass white dwarf stars are white dwarfs with stellar masses between 0.30~M$_{\odot}$ and 0.45~M$_{\odot}$ that show photometric variability due to gravity-mode pulsations. Within this mass range, they can harbour both a helium- and hybr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0185389dbd7307e0f92068b7bcef8e4b
Autor:
Maja Vučković, G. O. da Rosa, M. Uzundag, Keaton J. Bell, A. H. Córsico, Souza Oliveira Kepler, N. Reindl, Alina G. Istrate, Michael Higgins, Leandro Gabriel Althaus, Klaus Werner
Publikováno v:
Astronomy & Astrophysics, 655, 1-12
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Astronomy & Astrophysics, 655, pp. 1-12
Repositório Institucional da UFRGS
Universidade Federal do Rio Grande do Sul (UFRGS)
instacron:UFRGS
Astronomy & Astrophysics, 655, pp. 1-12
Context. The Transiting Exoplanet Survey Satellite (TESS) mission is revolutionizing the blossoming area of asteroseismology, particularly of pulsating white dwarfs and pre-white dwarfs, thus continuing the impulse of its predecessor, the Kepler miss
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d280c027d92cda65f9b6e66ce7e71c40
http://hdl.handle.net/2066/239752
http://hdl.handle.net/2066/239752
Autor:
Paulo C. C. Freire, Maurizio Salaris, C. Pallanca, Barbara Lanzoni, Jianxing Chen, Alina G. Istrate, M. Cadelano, Francesco R. Ferraro
Publikováno v:
The Astrophysical Journal, 905, 1-9
The Astrophysical Journal, 905, 1, pp. 1-9
The Astrophysical Journal, 905, 1, pp. 1-9
We report on the discovery of the companion star to the millisecond pulsar J1631+3627F in the globular cluster M13. By means of a combination of optical and near-UV high-resolution observations obtained with the Hubble Space Telescope, we identified
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f7fae0ed88292f558db623eacda11b5
http://arxiv.org/abs/2010.09740
http://arxiv.org/abs/2010.09740
Publikováno v:
Astronomy & Astrophysics, 645, pp. 1-27
Astronomy & Astrophysics, 645, 1-27
Astronomy & Astrophysics, 645, 1-27
Common-envelope (CE) evolution in massive binary systems is thought to be one of the most promising channels for the formation of compact binary mergers. In the case of merging binary black holes (BBHs), the essential CE phase takes place at a stage
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a91add56db6a71f49f6a5fe29a20a433
http://arxiv.org/abs/2006.11286
http://arxiv.org/abs/2006.11286
Autor:
Steven G. Parsons, Martin J. Dyer, A. J. Brown, D. I. Sahman, Vikram S. Dhillon, M. J. Green, Tom Marsh, S. P. Littlefair, Elmé Breedt, Alina G. Istrate, J. J. Hermes
Publikováno v:
Nature Astronomy, 4, 690-696
Nature Astronomy, 4, 7, pp. 690-696
Nature Astronomy, 4, 7, pp. 690-696
White dwarfs are the burnt out cores of Sun-like stars and are the final fate of 97% of all stars in our Galaxy. The internal structure and composition of white dwarfs are hidden by their high gravities, which causes all elements, apart from the ligh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::304456d49821e60b84a66daa071de4e0
http://arxiv.org/abs/2003.07371
http://arxiv.org/abs/2003.07371
Autor:
M. S. Kehl, A. Chalumeau, Kang Liu, Gilles Theureau, Lucas Guillemot, Ismaël Cognard, G. Desvignes, John Antoniadis, Norbert Wex, Lijing Shao, Alina G. Istrate, Thomas M. Tauris, Paulo C. C. Freire
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 499, 2, pp. 2276-2291
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 499 (2), pp.2276-2291. ⟨10.1093/mnras/staa2993⟩
Monthly Notices of the Royal Astronomical Society, 499, 2276-2291
Liu, K, Guillemot, L, Istrate, A G, Shao, L, Tauris, T M, Wex, N, Antoniadis, J, Chalumeau, A, Cognard, I, Desvignes, G, Freire, P C C, Kehl, M S & Theureau, G 2020, ' A revisit of PSR J1909-3744 with 15-yr high-precision timing ', Monthly Notices of the Royal Astronomical Society, vol. 499, no. 2, pp. 2276-2291 . https://doi.org/10.1093/mnras/staa2993
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 499 (2), pp.2276-2291. ⟨10.1093/mnras/staa2993⟩
Monthly Notices of the Royal Astronomical Society, 499, 2276-2291
Liu, K, Guillemot, L, Istrate, A G, Shao, L, Tauris, T M, Wex, N, Antoniadis, J, Chalumeau, A, Cognard, I, Desvignes, G, Freire, P C C, Kehl, M S & Theureau, G 2020, ' A revisit of PSR J1909-3744 with 15-yr high-precision timing ', Monthly Notices of the Royal Astronomical Society, vol. 499, no. 2, pp. 2276-2291 . https://doi.org/10.1093/mnras/staa2993
We report on a high-precision timing analysis and an astrophysical study of the binary millisecond pulsar, PSR J1909$-$3744, motivated by the accumulation of data with well improved quality over the past decade. Using 15 years of observations with th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d03b2c16de2937aa838d33a872d392e3
https://hdl.handle.net/2066/225644
https://hdl.handle.net/2066/225644
Publikováno v:
Astronomy & Astrophysics, 638, 1-19
Astronomy & Astrophysics, 638, pp. 1-19
Astronomy & Astrophysics, 638, pp. 1-19
Metallicity is known to significantly affect the radial expansion of a massive star: the lower the metallicity, the more compact the star, especially during its post-MS evolution. We study this effect in the context of binary evolution. Using the ste
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24feaa740940c83e6aaafbcec5828796
https://hdl.handle.net/https://repository.ubn.ru.nl/handle/2066/220201
https://hdl.handle.net/https://repository.ubn.ru.nl/handle/2066/220201
Autor:
Isaac D. Lopez, J. J. Hermes, Leila M. Calcaferro, Keaton J. Bell, Adam Samuels, Zachary P. Vanderbosch, Alejandro H. Córsico, Alina G. Istrate
Publikováno v:
The Astrophysical Journal, 922, 1-11
The Astrophysical Journal, 922, 2, pp. 1-11
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
The Astrophysical Journal, 922, 2, pp. 1-11
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We report the discovery of pulsations in the extremely low mass (ELM), likely helium-core white dwarf GD 278 via ground- and space-based photometry. GD 278 was observed by the Transiting Exoplanet Survey Satellite (TESS) in Sector 18 at a 2-min caden