Time-resolved HST UV echelle spectroscopy of IX Vel

L.E. Hartley; J.E. Drew; K.S. Long

Time-resolved HST UV echelle spectroscopy of IX Vel

L.E. Hartley, J.E. Drew, K.S. Long

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Abstract

In the hydrodynamical line-driven disk wind models of Proga, Stone & Drew (1998) the mass loss rate is a strong function of the local luminosity. Also, the outflow is found to be subject to clumping, where the main source of driving radiation is the accretion disk. In order to test these predictions, we have obtained high resolution UV spectroscopy of the brightest novalike variable, IX Vel. These data have allowed us to examine the line profile structure in unprecedented detail.

Original language	English
Title of host publication	In: The Physics of Cataclysmic Variables and Related Objects - ASP Conf Series 261
Publisher	Astronomical Society of the Pacific
Pages	483-484
ISBN (Print)	978-1-58381-597-7, 1-58381-101-X
Publication status	Published - 2002

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title = "Time-resolved HST UV echelle spectroscopy of IX Vel",

abstract = "In the hydrodynamical line-driven disk wind models of Proga, Stone & Drew (1998) the mass loss rate is a strong function of the local luminosity. Also, the outflow is found to be subject to clumping, where the main source of driving radiation is the accretion disk. In order to test these predictions, we have obtained high resolution UV spectroscopy of the brightest novalike variable, IX Vel. These data have allowed us to examine the line profile structure in unprecedented detail.",

author = "L.E. Hartley and J.E. Drew and K.S. Long",

note = "Original paper can be found at: http://www.astrosociety.org/pubs/cs/253.html Copyright ASP",

year = "2002",

language = "English",

isbn = "978-1-58381-597-7",

pages = "483--484",

booktitle = "In: The Physics of Cataclysmic Variables and Related Objects - ASP Conf Series 261",

publisher = "Astronomical Society of the Pacific",

address = "United States",

}

TY - GEN

T1 - Time-resolved HST UV echelle spectroscopy of IX Vel

AU - Hartley, L.E.

AU - Drew, J.E.

AU - Long, K.S.

N1 - Original paper can be found at: http://www.astrosociety.org/pubs/cs/253.html Copyright ASP

PY - 2002

Y1 - 2002

N2 - In the hydrodynamical line-driven disk wind models of Proga, Stone & Drew (1998) the mass loss rate is a strong function of the local luminosity. Also, the outflow is found to be subject to clumping, where the main source of driving radiation is the accretion disk. In order to test these predictions, we have obtained high resolution UV spectroscopy of the brightest novalike variable, IX Vel. These data have allowed us to examine the line profile structure in unprecedented detail.

AB - In the hydrodynamical line-driven disk wind models of Proga, Stone & Drew (1998) the mass loss rate is a strong function of the local luminosity. Also, the outflow is found to be subject to clumping, where the main source of driving radiation is the accretion disk. In order to test these predictions, we have obtained high resolution UV spectroscopy of the brightest novalike variable, IX Vel. These data have allowed us to examine the line profile structure in unprecedented detail.

M3 - Conference contribution

SN - 978-1-58381-597-7

SN - 1-58381-101-X

SP - 483

EP - 484

BT - In: The Physics of Cataclysmic Variables and Related Objects - ASP Conf Series 261

PB - Astronomical Society of the Pacific

ER -

Time-resolved HST UV echelle spectroscopy of IX Vel

Abstract

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