What dominates the X-ray emission of Andromeda at E> 20 keV? New constraints from NuSTAR and Swift on a very bright, hard X-ray source

Mihoko Yukita; Andrew Ptak; Thomas Maccarone; Ann E Hornschemeier; Daniel R Wik; Katja Pottschmidt; Valsamo Antoniou; Frederick K Baganoff; Bret Lehmer; Andreas Zezas

What dominates the X-ray emission of Andromeda at E> 20 keV? New constraints from NuSTAR and Swift on a very bright, hard X-ray source

Mihoko Yukita, Andrew Ptak, Thomas Maccarone, Ann E Hornschemeier, Daniel R Wik, Katja Pottschmidt, Valsamo Antoniou, Frederick K Baganoff, Bret Lehmer, Andreas Zezas

Physics

Research output: Contribution to conference › Paper

Original language	English
State	Published - 2016

Cite this

@conference{19f40d9d79f94550a209bd440f48d10a,

title = "What dominates the X-ray emission of Andromeda at E> 20 keV? New constraints from NuSTAR and Swift on a very bright, hard X-ray source",

author = "Mihoko Yukita and Andrew Ptak and Thomas Maccarone and Hornschemeier, {Ann E} and Wik, {Daniel R} and Katja Pottschmidt and Valsamo Antoniou and Baganoff, {Frederick K} and Bret Lehmer and Andreas Zezas",

year = "2016",

language = "English",

}

TY - CONF

T1 - What dominates the X-ray emission of Andromeda at E> 20 keV? New constraints from NuSTAR and Swift on a very bright, hard X-ray source

AU - Yukita, Mihoko

AU - Ptak, Andrew

AU - Maccarone, Thomas

AU - Hornschemeier, Ann E

AU - Wik, Daniel R

AU - Pottschmidt, Katja

AU - Antoniou, Valsamo

AU - Baganoff, Frederick K

AU - Lehmer, Bret

AU - Zezas, Andreas

PY - 2016

Y1 - 2016

M3 - Paper

ER -

What dominates the X-ray emission of Andromeda at E> 20 keV? New constraints from NuSTAR and Swift on a very bright, hard X-ray source

Fingerprint

Cite this