The broad Fe K line in MCG-6-30-15: results from the second ASCA long-look

K. Iwasawa; A. C. Fabian; A. J. Young

doi:10.1002/1521-3994(199908)320:4/5<244::AID-ASNA244>3.0.CO;2-#

The broad Fe K line in MCG-6-30-15: results from the second ASCA long-look

K. Iwasawa, A. C. Fabian, A. J. Young

School of Physics

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Abstract

We report results on the broad iron emission line of the Seyfert galaxy MCG-6-30-15, obtained from the second long ASCA observation in 1997. The time-averaged profile of the broad line is very similar to that seen with ASCA in 1994. A bright flare is seen in the light curve, during which the emission line peaks around 5 keV and most of its emission is shifted below 6 keV with no component detected at 6.4 keV (EW

Original language	English
Pages (from-to)	244
Journal	Astronomische Nachrichten
Volume	320
DOIs	https://doi.org/10.1002/1521-3994(199908)320:4/5<244::AID-ASNA244>3.0.CO;2-#
Publication status	Published - 1999

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http://adsabs.harvard.edu/abs/1999AN....320..244I

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title = "The broad Fe K line in MCG-6-30-15: results from the second ASCA long-look",

abstract = "We report results on the broad iron emission line of the Seyfert galaxy MCG-6-30-15, obtained from the second long ASCA observation in 1997. The time-averaged profile of the broad line is very similar to that seen with ASCA in 1994. A bright flare is seen in the light curve, during which the emission line peaks around 5 keV and most of its emission is shifted below 6 keV with no component detected at 6.4 keV (EW",

author = "K. Iwasawa and Fabian, \{A. C.\} and Young, \{A. J.\}",

year = "1999",

doi = "10.1002/1521-3994(199908)320:4/5<244::AID-ASNA244>3.0.CO;2-\#",

language = "English",

volume = "320",

pages = "244",

journal = "Astronomische Nachrichten",

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TY - JOUR

T1 - The broad Fe K line in MCG-6-30-15: results from the second ASCA long-look

AU - Iwasawa, K.

AU - Fabian, A. C.

AU - Young, A. J.

PY - 1999

Y1 - 1999

N2 - We report results on the broad iron emission line of the Seyfert galaxy MCG-6-30-15, obtained from the second long ASCA observation in 1997. The time-averaged profile of the broad line is very similar to that seen with ASCA in 1994. A bright flare is seen in the light curve, during which the emission line peaks around 5 keV and most of its emission is shifted below 6 keV with no component detected at 6.4 keV (EW

AB - We report results on the broad iron emission line of the Seyfert galaxy MCG-6-30-15, obtained from the second long ASCA observation in 1997. The time-averaged profile of the broad line is very similar to that seen with ASCA in 1994. A bright flare is seen in the light curve, during which the emission line peaks around 5 keV and most of its emission is shifted below 6 keV with no component detected at 6.4 keV (EW

U2 - 10.1002/1521-3994(199908)320:4/5<244::AID-ASNA244>3.0.CO;2-#

DO - 10.1002/1521-3994(199908)320:4/5<244::AID-ASNA244>3.0.CO;2-#

M3 - Article (Academic Journal)

SN - 0004-6337

VL - 320

SP - 244

JO - Astronomische Nachrichten

JF - Astronomische Nachrichten

ER -

The broad Fe K line in MCG-6-30-15: results from the second ASCA long-look

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