Skip to main content

Research Repository

See what's under the surface

Advanced Search

Evidence for Dynamically Driven Formation of the GW170817 Neutron Star Binary in NGC 4993

Palmese, A.; Hartley, W.; Tarsitano, F.; Conselice, Christopher J.; Lahav, O.; Allam, S.; Annis, J.; Lin, H.; Soares-Santos, M.; Tucker, D.; Brout, D.; Banerji, M.; Bechtol, K.; Diehl, H.T.; Fruchter, A.; García-Bellido, J.; Herner, K.; Levan, A.J.; Li, T.S.; Lidman, C.; Misra, K.; Sako, M.; Scolnic, D.; Smith, M.; Abbott, T.M.C.; Abdalla, F.B.; Benoit-Lévy, A.; Bertin, E.; Brooks, D.; Buckley-Geer, E.; Rosell, A. Carnero; Kind, M. Carrasco; Carretero, J.; Castander, F.J.; Cunha, C.E.; D’Andrea, C.B.; da Costa, L.N.; Davis, C.; DePoy, D.L.; Desai, S.; Dietrich, J.P.; Doel, P.; Drlica-Wagner, A.; Eifler, T.F.; Evrard, A.E.; Flaugher, B.; Fosalba, P.; Frieman, J.; Gaztanaga, E.; Gerdes, D.W.; Giannantonio, T.; Gruen, D.; Gruendl, R.A.; Gschwend, J.; Gutierrez, G.; Honscheid, K.; Jain, B.; James, D.J.; Jeltema, T.; Johnson, M.W.G.; Johnson, M.D.; Krause, E.; Kron, R.; Kuehn, K.; Kuhlmann, S.; Kuropatkin, N.; Lima, M.; Maia, M.A.G.; March, M.; Marshall, J.L.; McMahon, R.G.; Menanteau, F.; Miller, C.J.; Miquel, R.; Neilsen, E.; Ogando, R.L.C.; Plazas, A.A.; Reil, K.; Romer, A.K.; Sanchez, E.; Schindler, R.; Smith, R.C.; Sobreira, F.; Suchyta, E.; Swanson, M.E.C.; Tarle, G.; Thomas, D.; Thomas, R.C.; Walker, A.R.; Weller, J.; Zhang, Y.; Zuntz, J.

Authors

A. Palmese

W. Hartley

F. Tarsitano

Christopher J. Conselice

O. Lahav

S. Allam

J. Annis

H. Lin

M. Soares-Santos

D. Tucker

D. Brout

M. Banerji

K. Bechtol

H.T. Diehl

A. Fruchter

J. García-Bellido

K. Herner

A.J. Levan

T.S. Li

C. Lidman

K. Misra

M. Sako

D. Scolnic

M. Smith

T.M.C. Abbott

F.B. Abdalla

A. Benoit-Lévy

E. Bertin

D. Brooks

E. Buckley-Geer

A. Carnero Rosell

M. Carrasco Kind

J. Carretero

F.J. Castander

C.E. Cunha

C.B. D’Andrea

L.N. da Costa

C. Davis

D.L. DePoy

S. Desai

J.P. Dietrich

P. Doel

A. Drlica-Wagner

T.F. Eifler

A.E. Evrard

B. Flaugher

P. Fosalba

J. Frieman

E. Gaztanaga

D.W. Gerdes

T. Giannantonio

D. Gruen

R.A. Gruendl

J. Gschwend

G. Gutierrez

K. Honscheid

B. Jain

D.J. James

T. Jeltema

M.W.G. Johnson

M.D. Johnson

E. Krause

R. Kron

K. Kuehn

S. Kuhlmann

N. Kuropatkin

M. Lima

M.A.G. Maia

M. March

J.L. Marshall

R.G. McMahon

F. Menanteau

C.J. Miller

R. Miquel

E. Neilsen

R.L.C. Ogando

A.A. Plazas

K. Reil

A.K. Romer

E. Sanchez

R. Schindler

R.C. Smith

F. Sobreira

E. Suchyta

M.E.C. Swanson

G. Tarle

D. Thomas

R.C. Thomas

A.R. Walker

J. Weller

Y. Zhang

J. Zuntz



Abstract

We present a study of NGC 4993, the host galaxy of the GW170817 gravitational-wave event, the GRB 170817A short gamma-ray burst (sGRB), and the AT 2017gfo kilonova. We use Dark Energy Camera imaging, AAT spectra, and publicly available data, relating our findings to binary neutron star (BNS) formation scenarios and merger delay timescales. NGC 4993 is a nearby early-type galaxy, with an i-band Sérsic index n = 4.0 and low asymmetry (A = 0.04 ± 0.01). These properties are unusual for sGRB hosts. However, NGC 4993 presents shell-like structures and dust lanes indicative of a recent galaxy merger, with the optical transient located close to a shell. We constrain the star formation history (SFH) of the galaxy assuming that the galaxy merger produced a star formation burst, but find little to no ongoing star formation in either spatially resolved broadband SED or spectral fitting. We use the best-fit SFH to estimate the BNS merger rate in this type of galaxy, as ${R}_{\mathrm{NSM}}^{\mathrm{gal}}={5.7}_{-3.3}^{+0.57}\times {10}^{-6}{\mathrm{yr}}^{-1}$. If star formation is the only considered BNS formation scenario, the expected number of BNS mergers from early-type galaxies detectable with LIGO during its first two observing seasons is ${0.038}_{-0.022}^{+0.004}$, as opposed to ~0.5 from all galaxy types. Hypothesizing that the binary formed due to dynamical interactions during the galaxy merger, the subsequent time elapsed can constrain the delay time of the BNS coalescence. By using velocity dispersion estimates and the position of the shells, we find that the galaxy merger occurred t mer lesssim 200 Myr prior to the BNS coalescence.

Journal Article Type Article
Publication Date Nov 9, 2017
Journal The Astrophysical Journal
Print ISSN 2041-8205
Electronic ISSN 2041-8213
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 849
Issue 2
Article Number L34
APA6 Citation Palmese, A., Hartley, W., Tarsitano, F., Conselice, C. J., Lahav, O., Allam, S., …Zuntz, J. (2017). Evidence for Dynamically Driven Formation of the GW170817 Neutron Star Binary in NGC 4993. Astrophysical Journal Letters, 849(2), https://doi.org/10.3847/2041-8213/aa9660
DOI https://doi.org/10.3847/2041-8213/aa9660
Keywords galaxies: individual (NGC 4993); galaxies: evolution; galaxies: structure – gravitational waves
Publisher URL http://iopscience.iop.org/article/10.3847/2041-8213/aa9660/meta
Copyright Statement Copyright information regarding this work can be found at the following address: http://eprints.nottingh.../end_user_agreement.pdf
Additional Information © 2017. The American Astronomical Society. All rights reserved.

Files

Palmese_2017_ApJL_849_L34.pdf (1.2 Mb)
PDF

Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf





You might also like



Downloadable Citations

;