Exploring the high frequency emission of radio loud X-ray binaries

We report millimetre-wave continuum observations of the X-ray binaries Cygnus X-3, SS 433, LSI+61°303, Cygnus X-1 and GRS 1915+105. The observations were carried out with the IRAM 30 m-antenna at 250 GHz (1.25 mm) from 1998 March 14 to March 20. These millimetre measurements are complemented with ce...

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Autores principales:	Paredes, J.M., Martí, J., Peracaula, M., Pooley, G., Mirabel, I.F.
Formato:	JOUR
Materias:	Radio continuum: stars Stars: individual: Cygnus X-1 Stars: individual: Cygnus X-3 Stars: individual: GRS 1915+105 Stars: individual: LSI+61°303 Stars: individual: SS 433
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v357_n2_p507_Paredes
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

id	todo:paper_00046361_v357_n2_p507_Paredes
record_format	dspace
spelling	todo:paper_00046361_v357_n2_p507_Paredes2023-10-03T13:59:55Z Exploring the high frequency emission of radio loud X-ray binaries Paredes, J.M. Martí, J. Peracaula, M. Pooley, G. Mirabel, I.F. Radio continuum: stars Stars: individual: Cygnus X-1 Stars: individual: Cygnus X-3 Stars: individual: GRS 1915+105 Stars: individual: LSI+61°303 Stars: individual: SS 433 We report millimetre-wave continuum observations of the X-ray binaries Cygnus X-3, SS 433, LSI+61°303, Cygnus X-1 and GRS 1915+105. The observations were carried out with the IRAM 30 m-antenna at 250 GHz (1.25 mm) from 1998 March 14 to March 20. These millimetre measurements are complemented with centimetre observations from the Ryle Telescope, at 15 GHz (2.0 cm), and from the Green Bank Interferometer at 2.25 and 8.3 GHz (13 and 3.6 cm). Both Cygnus X-3 and SS 433 underwent moderate flaring events during our observations, whose main spectral evolution properties are described and interpreted. A significant spectral steepening was observed in both sources during the flare decay, that is likely to be caused by adiabatic expansion, inverse Compton and synchrotron losses. Finally, we also report 250 GHz upper limits for three additional undetected X-ray binary stars: LSI+65°010, LSI+61°235 and X Per. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00046361_v357_n2_p507_Paredes
institution	Universidad de Buenos Aires
institution_str	I-28
repository_str	R-134
collection	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic	Radio continuum: stars Stars: individual: Cygnus X-1 Stars: individual: Cygnus X-3 Stars: individual: GRS 1915+105 Stars: individual: LSI+61°303 Stars: individual: SS 433
spellingShingle	Radio continuum: stars Stars: individual: Cygnus X-1 Stars: individual: Cygnus X-3 Stars: individual: GRS 1915+105 Stars: individual: LSI+61°303 Stars: individual: SS 433 Paredes, J.M. Martí, J. Peracaula, M. Pooley, G. Mirabel, I.F. Exploring the high frequency emission of radio loud X-ray binaries
topic_facet	Radio continuum: stars Stars: individual: Cygnus X-1 Stars: individual: Cygnus X-3 Stars: individual: GRS 1915+105 Stars: individual: LSI+61°303 Stars: individual: SS 433
description	We report millimetre-wave continuum observations of the X-ray binaries Cygnus X-3, SS 433, LSI+61°303, Cygnus X-1 and GRS 1915+105. The observations were carried out with the IRAM 30 m-antenna at 250 GHz (1.25 mm) from 1998 March 14 to March 20. These millimetre measurements are complemented with centimetre observations from the Ryle Telescope, at 15 GHz (2.0 cm), and from the Green Bank Interferometer at 2.25 and 8.3 GHz (13 and 3.6 cm). Both Cygnus X-3 and SS 433 underwent moderate flaring events during our observations, whose main spectral evolution properties are described and interpreted. A significant spectral steepening was observed in both sources during the flare decay, that is likely to be caused by adiabatic expansion, inverse Compton and synchrotron losses. Finally, we also report 250 GHz upper limits for three additional undetected X-ray binary stars: LSI+65°010, LSI+61°235 and X Per.
format	JOUR
author	Paredes, J.M. Martí, J. Peracaula, M. Pooley, G. Mirabel, I.F.
author_facet	Paredes, J.M. Martí, J. Peracaula, M. Pooley, G. Mirabel, I.F.
author_sort	Paredes, J.M.
title	Exploring the high frequency emission of radio loud X-ray binaries
title_short	Exploring the high frequency emission of radio loud X-ray binaries
title_full	Exploring the high frequency emission of radio loud X-ray binaries
title_fullStr	Exploring the high frequency emission of radio loud X-ray binaries
title_full_unstemmed	Exploring the high frequency emission of radio loud X-ray binaries
title_sort	exploring the high frequency emission of radio loud x-ray binaries
url	http://hdl.handle.net/20.500.12110/paper_00046361_v357_n2_p507_Paredes
work_keys_str_mv	AT paredesjm exploringthehighfrequencyemissionofradioloudxraybinaries AT martij exploringthehighfrequencyemissionofradioloudxraybinaries AT peracaulam exploringthehighfrequencyemissionofradioloudxraybinaries AT pooleyg exploringthehighfrequencyemissionofradioloudxraybinaries AT mirabelif exploringthehighfrequencyemissionofradioloudxraybinaries
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Exploring the high frequency emission of radio loud X-ray binaries

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