The Fundamental Plane of Massive Quiescent Galaxies at z similar to 2

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The Fundamental Plane of Massive Quiescent Galaxies at z similar to 2. / Stockmann, Mikkel; Jorgensen, Inger; Toft, Sune; Conselice, Christopher J.; Faisst, Andreas; Margalef-Bentabol, Berta; Gallazzi, Anna; Zibetti, Stefano; Brammer, Gabriel B.; Gomez-Guijarro, Carlos; Hirschmann, Michaela; Lagos, Claudia D.; Valentino, Francesco M.; Zabl, Johannes.

In: Astrophysical Journal, Vol. 908, No. 2, 135, 01.02.2021.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Stockmann, M, Jorgensen, I, Toft, S, Conselice, CJ, Faisst, A, Margalef-Bentabol, B, Gallazzi, A, Zibetti, S, Brammer, GB, Gomez-Guijarro, C, Hirschmann, M, Lagos, CD, Valentino, FM & Zabl, J 2021, 'The Fundamental Plane of Massive Quiescent Galaxies at z similar to 2', Astrophysical Journal, vol. 908, no. 2, 135. https://doi.org/10.3847/1538-4357/abce66

APA

Stockmann, M., Jorgensen, I., Toft, S., Conselice, C. J., Faisst, A., Margalef-Bentabol, B., Gallazzi, A., Zibetti, S., Brammer, G. B., Gomez-Guijarro, C., Hirschmann, M., Lagos, C. D., Valentino, F. M., & Zabl, J. (2021). The Fundamental Plane of Massive Quiescent Galaxies at z similar to 2. Astrophysical Journal, 908(2), [135]. https://doi.org/10.3847/1538-4357/abce66

Vancouver

Stockmann M, Jorgensen I, Toft S, Conselice CJ, Faisst A, Margalef-Bentabol B et al. The Fundamental Plane of Massive Quiescent Galaxies at z similar to 2. Astrophysical Journal. 2021 Feb 1;908(2). 135. https://doi.org/10.3847/1538-4357/abce66

Author

Stockmann, Mikkel ; Jorgensen, Inger ; Toft, Sune ; Conselice, Christopher J. ; Faisst, Andreas ; Margalef-Bentabol, Berta ; Gallazzi, Anna ; Zibetti, Stefano ; Brammer, Gabriel B. ; Gomez-Guijarro, Carlos ; Hirschmann, Michaela ; Lagos, Claudia D. ; Valentino, Francesco M. ; Zabl, Johannes. / The Fundamental Plane of Massive Quiescent Galaxies at z similar to 2. In: Astrophysical Journal. 2021 ; Vol. 908, No. 2.

Bibtex

@article{c70f7a07991a4e81b2b5b4899f0b50e0,
title = "The Fundamental Plane of Massive Quiescent Galaxies at z similar to 2",
abstract = "We examine the Fundamental Plane (FP) and mass-to-light ratio (M/L) scaling relations using the largest sample of massive quiescent galaxies at 1.5 z <2.5 to date. The FP (r(e), sigma(e), I-e) is established using 19 UVJ quiescent galaxies from COSMOS with Hubble Space Telescope H-F160W rest-frame optical sizes and X-shooter absorption line-measured stellar velocity dispersions. For a very massive, log (M-*/M-circle dot) >11.26, subset of eight quiescent galaxies at z > 2, from Stockmann et al., we show that they cannot passively evolve to the local Coma cluster relation alone and must undergo significant structural evolution to mimic the sizes of local massive galaxies. The evolution of the FP and M/L scaling relations, from z = 2 to present day, for this subset are consistent with passive aging of the stellar population and minor merger structural evolution into the most massive galaxies in the Coma cluster and other massive elliptical galaxies from the MASSIVE Survey. Modeling the luminosity evolution from minor merger-added stellar populations favors a history of merging with {"}dry{"} quiescent galaxies.",
author = "Mikkel Stockmann and Inger Jorgensen and Sune Toft and Conselice, {Christopher J.} and Andreas Faisst and Berta Margalef-Bentabol and Anna Gallazzi and Stefano Zibetti and Brammer, {Gabriel B.} and Carlos Gomez-Guijarro and Michaela Hirschmann and Lagos, {Claudia D.} and Valentino, {Francesco M.} and Johannes Zabl",
year = "2021",
month = feb,
day = "1",
doi = "10.3847/1538-4357/abce66",
language = "English",
volume = "908",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - The Fundamental Plane of Massive Quiescent Galaxies at z similar to 2

AU - Stockmann, Mikkel

AU - Jorgensen, Inger

AU - Toft, Sune

AU - Conselice, Christopher J.

AU - Faisst, Andreas

AU - Margalef-Bentabol, Berta

AU - Gallazzi, Anna

AU - Zibetti, Stefano

AU - Brammer, Gabriel B.

AU - Gomez-Guijarro, Carlos

AU - Hirschmann, Michaela

AU - Lagos, Claudia D.

AU - Valentino, Francesco M.

AU - Zabl, Johannes

PY - 2021/2/1

Y1 - 2021/2/1

N2 - We examine the Fundamental Plane (FP) and mass-to-light ratio (M/L) scaling relations using the largest sample of massive quiescent galaxies at 1.5 z <2.5 to date. The FP (r(e), sigma(e), I-e) is established using 19 UVJ quiescent galaxies from COSMOS with Hubble Space Telescope H-F160W rest-frame optical sizes and X-shooter absorption line-measured stellar velocity dispersions. For a very massive, log (M-*/M-circle dot) >11.26, subset of eight quiescent galaxies at z > 2, from Stockmann et al., we show that they cannot passively evolve to the local Coma cluster relation alone and must undergo significant structural evolution to mimic the sizes of local massive galaxies. The evolution of the FP and M/L scaling relations, from z = 2 to present day, for this subset are consistent with passive aging of the stellar population and minor merger structural evolution into the most massive galaxies in the Coma cluster and other massive elliptical galaxies from the MASSIVE Survey. Modeling the luminosity evolution from minor merger-added stellar populations favors a history of merging with "dry" quiescent galaxies.

AB - We examine the Fundamental Plane (FP) and mass-to-light ratio (M/L) scaling relations using the largest sample of massive quiescent galaxies at 1.5 z <2.5 to date. The FP (r(e), sigma(e), I-e) is established using 19 UVJ quiescent galaxies from COSMOS with Hubble Space Telescope H-F160W rest-frame optical sizes and X-shooter absorption line-measured stellar velocity dispersions. For a very massive, log (M-*/M-circle dot) >11.26, subset of eight quiescent galaxies at z > 2, from Stockmann et al., we show that they cannot passively evolve to the local Coma cluster relation alone and must undergo significant structural evolution to mimic the sizes of local massive galaxies. The evolution of the FP and M/L scaling relations, from z = 2 to present day, for this subset are consistent with passive aging of the stellar population and minor merger structural evolution into the most massive galaxies in the Coma cluster and other massive elliptical galaxies from the MASSIVE Survey. Modeling the luminosity evolution from minor merger-added stellar populations favors a history of merging with "dry" quiescent galaxies.

U2 - 10.3847/1538-4357/abce66

DO - 10.3847/1538-4357/abce66

M3 - Journal article

VL - 908

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 135

ER -

ID: 257746789