Zobrazeno 1 - 10
of 25
pro vyhledávání: '"Swayne, Matthew"'
Autor:
Davis, Yasmin T., Triaud, Amaury H. M. J., Freckelton, Alix V., Mortier, Annelies, Sebastian, Daniel, Baycroft, Thomas, Brahm, Rafael, Dransfield, Georgina, Duck, Alison, Henning, Thomas, Hobson, Melissa J., Jordán, Andrés, Kunovac, Vedad, Martin, David V., Maxted, Pierre F. L., Sairam, Lalitha, Standing, Matthew R., Swayne, Matthew I., Trifonov, Trifon, Udry, Stéphane
In the hunt for Earth-like exoplanets it is crucial to have reliable host star parameters, as they have a direct impact on the accuracy and precision of the inferred parameters for any discovered exoplanet. For stars with masses between 0.35 and 0.5
Externí odkaz:
http://arxiv.org/abs/2312.09156
Autor:
Duck, Alison, Martin, David V., Gill, Sam, Armitage, Tayt, Martínez, Romy Rodríguez, Maxted, Pierre F. L., Sebastian, Daniel, Sethi, Ritika, Swayne, Matthew I., Cameron, Andrew Collier, Dransfield, Georgina, Gaudi, B. Scott, Gillon, Michael, Hellier, Coel, Kunovac, Vedad, Lovis, Christophe, McCormac, James, Pepe, Francesco A., Pollacco, Don, Sairam, Lalitha, Santerne, Alexandre, Ségransan, Damien, Standing, Matthew R., Southworth, John, Triaud, Amaury H. M. J., Udry, Stephane
M-dwarfs are the most abundant stars in the galaxy and popular targets for exoplanet searches. However, their intrinsic faintness and complex spectra inhibit precise characterisation. We only know of dozens of M-dwarfs with fundamental parameters of
Externí odkaz:
http://arxiv.org/abs/2208.10534
Autor:
Martin, David V., Armitage, Tayt, Duck, Alison, Swayne, Matthew I., Martínez, Romy Rodríguez, Sethi, Ritika, Gaudi, B. Scott, Gill, Sam, Sebastian, Daniel, Maxted, Pierre F. L.
Well-characterised M-dwarfs are rare, particularly with respect to effective temperature. In this letter we re-analyse two benchmark M-dwarfs in eclipsing binaries from Kepler/K2: KIC 1571511AB and HD 24465AB. Both have temperatures reported to be ho
Externí odkaz:
http://arxiv.org/abs/2208.10510
Publikováno v:
MNRAS: Letters, 498(1), (2020), L15-L19
A 2014 study of the eclipsing binary star 1SWASPJ011351.29+314909.7 (J0113+31) reported an unexpectedly high effective temperature for the M-dwarf companion to the 0.95-M$_{\odot}$ primary star. The effective temperature inferred from the secondary e
Externí odkaz:
http://arxiv.org/abs/2007.04653
Akademický článek
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Autor:
Taquet, Vianney, van Dishoeck, Ewine F., Swayne, Matthew, Harsono, Daniel, Jørgensen, Jes K., Maud, Luke, Ligterink, Niels F. W., Müller, Holger S. P., Codella, Claudio, Altwegg, Kathrin, Bieler, Andre, Coutens, Audrey, Drozdovskaya, Maria N., Furuya, Kenji, Persson, Magnus V., Hoff, Merel L. R. van 't, Walsh, Catherine, Wampfler, Suzanne F.
Recent measurements carried out at comet 67P/C-G with the ${\it Rosetta}$ probe revealed that molecular oxygen, O$_2$, is the fourth most abundant molecule in comets. Models show that O$_2$ is likely of primordial nature, coming from the interstellar
Externí odkaz:
http://arxiv.org/abs/1805.12492
Akademický článek
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Akademický článek
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Autor:
Sebastian, Daniel, Swayne, Matthew, Maxted, Pierre F.L., Triaud, Amaury H.M.J., Sousa, Sérgio G., Olofsson, Göran, Beck, Mathias, Billot, Nicolas, Hoyer, Sergio, Gill, S., Heidari, N., Martin, David V., Persson, M., Standing, Matthew R., Alibert, Yann, Alonso, Roi, Anglada, Guillem, Asquier, J., Bárczy, Tamás, Barrado, David, Queloz, Didier, et. al.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 519 (3)
Eclipsing binaries are important benchmark objects to test and calibrate stellar structure and evolution models. This is especially true for binaries with a fully convective M-dwarf component for which direct measurements of these stars’ masses and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9702f94fd205d00fc6daffa10bf895d0
https://hdl.handle.net/20.500.11850/615129
https://hdl.handle.net/20.500.11850/615129
Autor:
Swayne, Matthew, Maxted, Pierre
There are numerous examples in the literature of low-mass stars (
{"references":["Charbonneau D., Deming D., 2007, preprint (arXiv:0706.1047)","Quirrenbach A. et al., 2014, in Ramsay S. K., McLean I. S., Takami H., eds, SPIE Conf. Ser. Vol. 9147
{"references":["Charbonneau D., Deming D., 2007, preprint (arXiv:0706.1047)","Quirrenbach A. et al., 2014, in Ramsay S. K., McLean I. S., Takami H., eds, SPIE Conf. Ser. Vol. 9147
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7bbbfa2cf9c0008761b255dbd592fa52