Zobrazeno 1 - 10
of 111
pro vyhledávání: '"Nicole St Louis"'
Autor:
Noel D. Richardson, Konstanze Zwintz, Anthony F. J. Moffat, Adam Popowicz, Nour Ibrahim, Herbert Pablo, Nicole St-Louis, Gerald Handler, Catherine Lovekin, Dominic M. Bowman, Gregg A. Wade, Ashley Elliott
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 509:4246-4255
Luminous Blue Variables (LBVs) are massive stars that are likely to be a transitionary phase between O stars and hydrogen-free classical Wolf–Rayet stars. The variability of these stars has been an area of study for both professional and amateur as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d304cb43c307e957a83deb82a073be43
https://doi.org/10.1093/mnras/stab3112
https://doi.org/10.1093/mnras/stab3112
Autor:
Geraldine J. Peters, Kenneth G. Gayley, Richard Ignace, Carol E. Jones, Yaël Nazé, Nicole St-Louis, Heloise Stevance, Jorick S. Vink, Noel D. Richardson, Jennifer L. Hoffman, Jamie R. Lomax, Tomer Shenar, Andrew G. Fullard, Paul A. Scowen
Publikováno v:
Astrophysics and Space Science, 367(12):119. Springer Netherlands
One objective of the Polstar spectropolarimetry mission is to characterize the degree of nonconservative mass transfer that occurs at various stages of binary evolution, from the initial mass reversal to the late Algol phase. The proposed instrument
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::268847bc36c3758f5984ff13ca08d021
https://dare.uva.nl/personal/pure/en/publications/ultraviolet-spectropolarimetry(f558863d-b43f-4c3f-849d-f5f6bc7c8afd).html
https://dare.uva.nl/personal/pure/en/publications/ultraviolet-spectropolarimetry(f558863d-b43f-4c3f-849d-f5f6bc7c8afd).html
Autor:
Kenneth G. Gayley, Jorick S. Vink, Asif ud-Doula, Alexandre David-Uraz, Richard Ignace, Raman Prinja, Nicole St-Louis, Sylvia Ekström, Yaël Nazé, Tomer Shenar, Paul A. Scowen, Natallia Sudnik, Stan P. Owocki, Jon O. Sundqvist, Florian A. Driessen, Levin Hennicker
Publikováno v:
Astrophysics and Space Science, 367(12):123. Springer Netherlands
The most massive stars are thought to lose a significant fraction of their mass in a steady wind during the main-sequence and blue supergiant phases. This in turn sets the stage for their further evolution and eventual supernova, and preconditions th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c3fca02297abbc677c2b0ea1dd024d16
https://doi.org/10.1007/s10509-022-04142-6
https://doi.org/10.1007/s10509-022-04142-6
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 506:4465-4472
Θ Mus = HD 113904 is a massive multiple system containing the WC5/6 + O6/7V binary WR48 in a $19.1\, \mathrm{ d}$ circular orbit. Previous attempts to constrain the variable photometric properties of this binary subsystem have been thwarted by the d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7481e807f9a738c73c63a6a37c62bdf4
https://doi.org/10.1093/mnras/stab1939
https://doi.org/10.1093/mnras/stab1939
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy IX.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::63397adfa699f941a7d593709b98f318
https://doi.org/10.1117/12.2627506
https://doi.org/10.1117/12.2627506
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 501:5350-5361
We present a detailed study of M1-67, a well-known nebula around the population I Wolf-Rayet star WR 124 (WNh 8), based on datacubes obtained with the imaging Fourier transform spectrometer SITELLE at the Canada-France-Hawaii Telescope (CFHT). This a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::45241e22be2ec8e786b7fabaee2777be
https://doi.org/10.1093/mnras/staa3971
https://doi.org/10.1093/mnras/staa3971
Autor:
R. Leadbeater, P. Stinner, Michael Potter, D. Weiss, B Gauza, E. Stinner, T. Moldenhawer, G. Grutzeck, A. F. J. Moffat, F. Bolduan, D. Fuchs, Johan H. Knapen, L. Schanne, Noel D. Richardson, D. Küsters, Deqing Li, Thomas Eversberg, Grant M. Hill, K. Strandbaek, Sergio Simón-Díaz, Filipe Marques Dias, A. Wendt, B. Kubátová, J. B. P. Strachan, M. Langenbrink, Nicole St-Louis, Caroline Piaulet, U. Waldschläger, Tomer Shenar, B. Mauclaire, H. Sieske, A. Lopez, D. P. Sablowski, T. Garrel, J. Schmidt, Berthold Stober, Jiří Kubát, D. Verilhac, E. M. dos Santos, T. Hunger, P. Dubreuil, T. Syder
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 497:4448-4458
We present the results of a four-month, spectroscopic campaign of the Wolf-Rayet dust-making binary, WR137. We detect only small-amplitude, random variability in the CIII5696 emission line and its integrated quantities (radial velocity, equivalent wi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5ee9ff3bda7a0b7b7484a2204e2a70f
https://doi.org/10.1093/mnras/staa2214
https://doi.org/10.1093/mnras/staa2214
Autor:
Richard Ignace, Andrew Fullard, Manisha Shrestha, Yaël Nazé, Kenneth Gayley, Jennifer L. Hoffman, Jamie R. Lomax, Nicole St-Louis
Massive star binaries are critical laboratories for measuring masses and stellar wind mass-loss rates. A major challenge is inferring viewing inclination and extracting information about the colliding wind interaction (CWI) region. Polarimetric varia
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a69c43ff02da69ef61bf39f0e954347b
WR22 = HD 92740 is a bright (V = 6.4 $mag$), intrinsically luminous, double-line WN7h + O9III-V binary exhibiting one sharp 8\% deep eclipse near periastron in its elliptical (e = 0.6) 80-day orbit, when the WR-star passes in front of the O star, wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::713f7d8e48bfc371fd4efa7c4f337efb
http://arxiv.org/abs/2111.09400
http://arxiv.org/abs/2111.09400
Autor:
Parmanand Maharaj, Ashton Ramsundar, Sushil Devarashetty, Leonardo Akan, Camille Greene, Elizabeth Persad, Vindra A Singh, Nirmala Hallai, Vanita Shukla, Nicole St Louis, Virendra Singh
Publikováno v:
Abstracts.
Background Sneddon syndrome is a rare, progressive small and medium-vessel vasculopathy characterized by the clinical occurrence of livedo racemosa and ischaemic cerebrovascular events. Objectives We present the clinical course and management of this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c16a1f702bc7ebedb5b618cbd6c17aa1
https://doi.org/10.1136/archdischild-2021-rcpch.68
https://doi.org/10.1136/archdischild-2021-rcpch.68