Repository logo
Log in(current)
Repository logoMIT Open ScholarshipDSpace@MIT
  1. Home
  2. MIT Open Access Articles
  3. MIT Open Access Articles
  4. NuSTAR Observations of X-Ray Binaries

NuSTAR Observations of X-Ray Binaries

Thumbnail Image
Download
Name

NuSTAR Observations.pdf

Size

170.4 KB

Format

Adobe PDF

Checksum (MD5)

1f7b75e64b1e8efffa2aee93ac8fe16e

Author(s)
Tomsick, John A.
•
Bellm, Eric
•
Fuerst, Felix
•
Harrison, Fiona
•
Miyasaka, Hiromasa
•
Tendulkar, Shriharsh
•
Bhalerao, Varun
•
King, Ashley
•
Natalucci, Lorenzo
•
Stern, Daniel
more
Date Issued
September 2014
Journal
10th INTEGRAL Workshop: "A Synergistic View of the High Ener gy Sky" - Integral2014, 15-19 September 2014 Annapolis, MD, USA
Citation
Tomsick, John A., Eric Bellm, Felix Fuerst, Fiona Harrison, Hiromasa Miyasak a, Shriharsh Tendulkar, Varun Bhalerao, Deepto Chakrabarty, Ashley King, Jon M. Miller, Lorenzo Natalucci and Daniel Stern. "NuSTAR Observations of X-Ray Binaries." Article from 10th INTEGRAL Workshop: "A Synergistic View of the High Energy Sky" - Integral2014, 15-19 September 2014 Annapolis, MD, USA.
Version
Final published version
Abstract
As of 2014 August, the Nuclear Spectroscopic Telescope Array (NuSTAR) had observed ~30 X-ray binaries either as part of the planned program, as targets of opportunity, or for instrument calibration. The main science goals for the observations include probing the inner part of the accretion disk and constraining black hole spins via reflection components, providing the first observations of hard X-ray emission from quiescent Low Mass X-ray Binaries (LMXBs), measuring cyclotron lines from accreting pulsars, and studying type I X-ray bursts from neutron stars. Here, we describe the science objectives in more depth and give an overview of the NuSTAR observations that have been carried out to achieve the objectives. These include observation of four "IGR" High Mass X-ray Binaries (HMXBs) discovered by INTEGRAL. We also summarize the results that have been obtained and their implications. Among the IGR HMXBs, we focus on the discovery of a cyclotron line in the spectrum of IGR J17544-2619.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Terms of Use
Creative Commons Attribution-Noncommercial-Share Alike
http://creativecommons.org/licenses/by-nc-sa/4.0/
Persistent DSpace Link
http://hdl.handle.net/1721.1/109115
DOI of Published Version
https://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=228
Repository logo
PrivacyPermissionsAccessibilityContact us
Repository logo
Notify us about copyright concerns.