Fading of low-mass X-ray binary Swift J1858.6-0814 to quiescence level

Payaswini Saikia; David Russell; M. C. Baglio; D. M. Bramich; F. Lewis

Fading of low-mass X-ray binary Swift J1858.6-0814 to quiescence level

Payaswini Saikia, David Russell, M. C. Baglio, D. M. Bramich, F. Lewis

Physics

Research output: Book/Report › Other report

Abstract

The low-mass X-ray binary Swift J1858.6-0814 has been in outburst since 2018 October 25 (MJD 58416; Krimm et al. ATel #12151). The source had a consistently hard X-ray spectrum, with a strong neutral iron K-alpha emission line, prominent X-ray variability and evidence for intrinsic absorption, and has been in this active state for more than a year (ATel #12158, #12220, #12512, #13255).

Original language	English (US)
Publisher	The Astronomer's Telegram
Number of pages	1
Volume	13719
State	Published - May 8 2020

Access to Document

Cite this

@book{31e5b53abdb54bee83d210361b57a669,

title = "Fading of low-mass X-ray binary Swift J1858.6-0814 to quiescence level",

abstract = "The low-mass X-ray binary Swift J1858.6-0814 has been in outburst since 2018 October 25 (MJD 58416; Krimm et al. ATel #12151). The source had a consistently hard X-ray spectrum, with a strong neutral iron K-alpha emission line, prominent X-ray variability and evidence for intrinsic absorption, and has been in this active state for more than a year (ATel #12158, #12220, #12512, #13255).",

author = "Payaswini Saikia and David Russell and Baglio, {M. C.} and Bramich, {D. M.} and F. Lewis",

year = "2020",

month = may,

day = "8",

language = "English (US)",

volume = "13719",

publisher = "The Astronomer's Telegram",

}

TY - BOOK

T1 - Fading of low-mass X-ray binary Swift J1858.6-0814 to quiescence level

AU - Saikia, Payaswini

AU - Russell, David

AU - Baglio, M. C.

AU - Bramich, D. M.

AU - Lewis, F.

PY - 2020/5/8

Y1 - 2020/5/8

N2 - The low-mass X-ray binary Swift J1858.6-0814 has been in outburst since 2018 October 25 (MJD 58416; Krimm et al. ATel #12151). The source had a consistently hard X-ray spectrum, with a strong neutral iron K-alpha emission line, prominent X-ray variability and evidence for intrinsic absorption, and has been in this active state for more than a year (ATel #12158, #12220, #12512, #13255).

AB - The low-mass X-ray binary Swift J1858.6-0814 has been in outburst since 2018 October 25 (MJD 58416; Krimm et al. ATel #12151). The source had a consistently hard X-ray spectrum, with a strong neutral iron K-alpha emission line, prominent X-ray variability and evidence for intrinsic absorption, and has been in this active state for more than a year (ATel #12158, #12220, #12512, #13255).

M3 - Other report

VL - 13719

BT - Fading of low-mass X-ray binary Swift J1858.6-0814 to quiescence level

PB - The Astronomer's Telegram

ER -

Fading of low-mass X-ray binary Swift J1858.6-0814 to quiescence level

Abstract

Access to Document

Fingerprint

Cite this