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pro vyhledávání: '"Trueba Nicolas"'
Autor:
Marengo Massimo, Neeley Jillian, Bono Giuseppe, Braga Vittorio, Dall’Ora Massimo, Marconi Marcella, Trueba Nicolas, Magurno Davide
Publikováno v:
EPJ Web of Conferences, Vol 152, p 07004 (2017)
We present our project to calibrate the RR Lyræ period-luminosity-metallicity relation using a sample of Galactic calibrators in the halo and globular clusters.
Externí odkaz:
https://doaj.org/article/e18d152ef0214054acaa371ecc23f6f5
Autor:
Trueba, Nicolas, Miller, J. M., Fabian, A. C., Kaastra, J., Kallman, T., Lohfink, A., Ludlam, R. M., Proga, D., Raymond, J., Reynolds, C., Reynolds, M., Zoghbi, A.
Analyses of absorption from disk winds and atmospheres in accreting compact objects typically treat the central emitting regions in these systems as point sources relative to the absorber. This assumption breaks down if the absorbing gas is located w
Externí odkaz:
http://arxiv.org/abs/2111.04764
Autor:
Trueba, Nicolas, Miller, J. M., Fabian, A. C., Kaastra, J., Kallman, T., Lohfink, A., Proga, D., Raymond, J., Reynolds, C., Reynolds, M., Zoghbi, A.
The very small accretion disks in ultra-compact X-ray binaries (UCXBs) are special laboratories in which to study disk accretion and outflows. We report on three sets of new (250 ks total) and archival (50 ks) Chandra/HETG observations of the "dippin
Externí odkaz:
http://arxiv.org/abs/2008.01083
Autor:
Trueba, Nicolas, Miller, J. M., Kaastra, J., Zoghbi, A., Kallman, A. C. Fabian T., Proga, D., Raymond, J.
The mechanisms that drive disk winds are a window into the physical processes that underlie the disk. Stellar-mass black holes are an ideal setting in which to explore these mechanisms, in part because their outbursts span a broad range in mass accre
Externí odkaz:
http://arxiv.org/abs/1910.11243
Autor:
Meng, Huan Y. A., Rieke, George, Dubois, Franky, Kennedy, Grant, Marengo, Massimo, Siegel, Michael, Su, Kate, Trueba, Nicolas, Wyatt, Mark, Boyajian, Tabetha, Lisse, C. M., Logie, Ludwig, Rau, Steve, Vanaverbeke, Sigfried
To test alternative hypotheses for the behavior of KIC 8462852, we obtained measurements of the star over a wide wavelength range from the UV to the mid-infrared from October 2015 through December 2016, using Swift, Spitzer and at AstroLAB IRIS. The
Externí odkaz:
http://arxiv.org/abs/1708.07556
Autor:
Neeley, Jillian R., Marengo, Massimo, Bono, Giuseppe, Braga, Vittorio F., Dall'Ora, Massimo, Magurno, Davide, Marconi, Marcella, Trueba, Nicolas, Tognelli, Emanuele, Moroni, Pier G. Prada, Beaton, Rachael L., Freedman, Wendy L., Madore, Barry F., Monson, Andrew J., Scowcroft, Victoria, Seibert, Mark, Stetson, Peter B.
We present new theoretical period-luminosity-metallicity (PLZ) relations for RR Lyrae stars (RRL) at Spitzer and WISE wavelengths. The PLZ relations were derived using nonlinear, time-dependent convective hydrodynamical models for a broad range in me
Externí odkaz:
http://arxiv.org/abs/1705.01970
Akademický článek
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Akademický článek
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Autor:
Trueba, Nicolas, Miller, J. M., Fabian, A. C., Kaastra, J., Kallman, T., Lohfink, A., Proga, D., Raymond, J., Reynolds, C., Reynolds, M., Zoghbi, A.
Publikováno v:
Astrophysical Journal Letters; 8/10/2020, Vol. 899 Issue 1, p1-12, 12p