On Its Way to the Neutron Star-White Dwarf Binary Graveyard, IGR J16194−2810, A First Ascent M Giant X-Ray Binary

Autor(en)
Kenneth H. Hinkle, Francis C. Fekel, Oscar Straniero, Zachary G. Maas, Richard R. Joyce, Thomas Lebzelter, Matthew W. Muterspaugh, James R. Sowell
Abstrakt

A single-lined spectroscopic orbit for the M giant in the X-ray binary IGR J16194−2810 is determined from a time series of optical spectra. The spectroscopic orbital period of 192.5 days is twice that of the photometric period, confirming that the M giant in the system is an ellipsoidal variable. The giant is identified as a first ascent giant approaching the red giant tip. The primary is a neutron star (NS) with its M giant companion filling its Roche lobe, verifying the system classification as a low-mass X-ray binary (LMXB). Stellar C, N, O, and Fe abundances are derived for the M giant with the C, N, and O values typical for a field giant with [Fe/H] = −0.14. The system does not have a large kick velocity. Models for the evolution of the system into a binary NS-white dwarf are presented. The X-ray properties are discussed in the context of this model. This binary is a rare example of a luminous, long orbital period LMXB early in the transient ellipsoidal phase.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Gemini Observatory Northern Operations Center, Tennessee State University, INAF - Osservatorio Astronomico d'Abruzzo, INAF-Osservatorio Astrofisico di Torino, Istituto Nazionale di Fisica Nucleare (INFN), Roma, Indiana University Bloomington, Columbia State Community College, Georgia Institute of Technology
Journal
Astrophysical Journal
Band
969
Anzahl der Seiten
22
ISSN
0004-637X
DOI
https://doi.org/10.3847/1538-4357/ad4641
Publikationsdatum
07-2024
Peer-reviewed
Ja
ÖFOS 2012
103003 Astronomie, 103004 Astrophysik
ASJC Scopus Sachgebiete
Astronomy and Astrophysics, Space and Planetary Science
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/453b5e6f-6de5-4644-98d8-0059aa70f8c0