A potential galaxy threshing system in the COSMOS field

S. S. Sasaki; Y. Taniguchi; N. Scoville; B. Mobasher; H. Aussel; D. B. Sanders; A. Koekemoer; M. Ajiki; Y. Komiyama; S. Miyazaki; N. Kaifu; H. Karoji; S. Okamura; N. Arimoto; K. Ohta; Y. Shioya; T. Murayama; T. Nagao; J. Koda; L. Hainline; A. Renzini; M. Giavalisco; O. Le Fèvre; C. Impey; M. Elvis; S. Lilly; M. Rich; E. Schinnerer; K. Sheth

doi:10.1086/516581

A potential galaxy threshing system in the COSMOS field

S. S. Sasaki
, Y. Taniguchi
, N. Scoville
, B. Mobasher
, H. Aussel
, D. B. Sanders
, A. Koekemoer
, M. Ajiki
, Y. Komiyama
, S. Miyazaki
, N. Kaifu
, H. Karoji
, S. Okamura
, N. Arimoto
, K. Ohta
, Y. Shioya
, T. Murayama
, T. Nagao
, J. Koda
, L. Hainline

A. Renzini, M. Giavalisco, O. Le Fèvre, C. Impey, M. Elvis, S. Lilly, M. Rich, E. Schinnerer, K. Sheth

Physics and Astronomy

Tohoku University
Ehime University
California Institute of Technology
University of Hawai'i at Mānoa
Space Telescope Science Institute
Université Paris VII
National Astronomical Observatory of Japan (NAOJ)
The University of Tokyo
Kyoto University
Osservatorio Astrofisico Di Arcetri, Florence
European Southern Observatory
LAM
University of Arizona
Harvard-Smithsonian Ctr. Astrophys.
Swiss Federal Institute of Technology Zurich
University of California at Los Angeles
Max Planck Institute for Astronomy

Research output: Contribution to journal › Article › peer-review

7 Scopus citations

Abstract

We report on the discovery of a new potential galaxy threshing system in the COSMOS 2 square degree field using the prime-focus camera, Suprime-Cam, on the 8.2 m Subaru Telescope. This system consists of a giant elliptical galaxy with M _v ≈ -21.6 and a tidally disrupted satellite galaxy with M _v PS -17.7 at a photometric redshift of z ≈ 0.08. This redshift is consistent with the spectroscopic redshift of 0.079 for the giant elliptical galaxy obtained from the Sloan Digital Sky Survey (SDSS) archive. The luminosity masses of the two galaxies are 3.7 × 10 ¹² and 3.7 × 10 ⁹ M _⊙, respectively. The distance between the two galaxies is greater than 100 kpc. The two tidal tails emanating from the satellite galaxy extend over 150 kpc. This system would be the second well-defined galaxy threshing system found so far.

Original language	English
Pages (from-to)	511-517
Number of pages	7
Journal	Astrophysical Journal, Supplement Series
Volume	172
Issue number	1
DOIs	https://doi.org/10.1086/516581
State	Published - 2007

Keywords

Galaxies: evolution
Galaxies: interactions

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10.1086/516581

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Sasaki, S. S., Taniguchi, Y., Scoville, N., Mobasher, B., Aussel, H., Sanders, D. B., Koekemoer, A., Ajiki, M., Komiyama, Y., Miyazaki, S., Kaifu, N., Karoji, H., Okamura, S., Arimoto, N., Ohta, K., Shioya, Y., Murayama, T., Nagao, T., Koda, J., ... Sheth, K. (2007). A potential galaxy threshing system in the COSMOS field. Astrophysical Journal, Supplement Series, 172(1), 511-517. https://doi.org/10.1086/516581

@article{735787f00fe94620b910f621ab726afd,

title = "A potential galaxy threshing system in the COSMOS field",

abstract = "We report on the discovery of a new potential galaxy threshing system in the COSMOS 2 square degree field using the prime-focus camera, Suprime-Cam, on the 8.2 m Subaru Telescope. This system consists of a giant elliptical galaxy with M v ≈ -21.6 and a tidally disrupted satellite galaxy with M v PS -17.7 at a photometric redshift of z ≈ 0.08. This redshift is consistent with the spectroscopic redshift of 0.079 for the giant elliptical galaxy obtained from the Sloan Digital Sky Survey (SDSS) archive. The luminosity masses of the two galaxies are 3.7 × 10 12 and 3.7 × 10 9 M ⊙, respectively. The distance between the two galaxies is greater than 100 kpc. The two tidal tails emanating from the satellite galaxy extend over 150 kpc. This system would be the second well-defined galaxy threshing system found so far.",

keywords = "Galaxies: evolution, Galaxies: interactions",

author = "Sasaki, \{S. S.\} and Y. Taniguchi and N. Scoville and B. Mobasher and H. Aussel and Sanders, \{D. B.\} and A. Koekemoer and M. Ajiki and Y. Komiyama and S. Miyazaki and N. Kaifu and H. Karoji and S. Okamura and N. Arimoto and K. Ohta and Y. Shioya and T. Murayama and T. Nagao and J. Koda and L. Hainline and A. Renzini and M. Giavalisco and \{Le F{\`e}vre\}, O. and C. Impey and M. Elvis and S. Lilly and M. Rich and E. Schinnerer and K. Sheth",

year = "2007",

doi = "10.1086/516581",

language = "English",

volume = "172",

pages = "511--517",

journal = "Astrophysical Journal, Supplement Series",

issn = "0067-0049",

number = "1",

}

Sasaki, SS, Taniguchi, Y, Scoville, N, Mobasher, B, Aussel, H, Sanders, DB, Koekemoer, A, Ajiki, M, Komiyama, Y, Miyazaki, S, Kaifu, N, Karoji, H, Okamura, S, Arimoto, N, Ohta, K, Shioya, Y, Murayama, T, Nagao, T, Koda, J, Hainline, L, Renzini, A, Giavalisco, M, Le Fèvre, O, Impey, C, Elvis, M, Lilly, S, Rich, M, Schinnerer, E & Sheth, K 2007, 'A potential galaxy threshing system in the COSMOS field', Astrophysical Journal, Supplement Series, vol. 172, no. 1, pp. 511-517. https://doi.org/10.1086/516581

TY - JOUR

T1 - A potential galaxy threshing system in the COSMOS field

AU - Sasaki, S. S.

AU - Taniguchi, Y.

AU - Scoville, N.

AU - Mobasher, B.

AU - Aussel, H.

AU - Sanders, D. B.

AU - Koekemoer, A.

AU - Ajiki, M.

AU - Komiyama, Y.

AU - Miyazaki, S.

AU - Kaifu, N.

AU - Karoji, H.

AU - Okamura, S.

AU - Arimoto, N.

AU - Ohta, K.

AU - Shioya, Y.

AU - Murayama, T.

AU - Nagao, T.

AU - Koda, J.

AU - Hainline, L.

AU - Renzini, A.

AU - Giavalisco, M.

AU - Le Fèvre, O.

AU - Impey, C.

AU - Elvis, M.

AU - Lilly, S.

AU - Rich, M.

AU - Schinnerer, E.

AU - Sheth, K.

PY - 2007

Y1 - 2007

N2 - We report on the discovery of a new potential galaxy threshing system in the COSMOS 2 square degree field using the prime-focus camera, Suprime-Cam, on the 8.2 m Subaru Telescope. This system consists of a giant elliptical galaxy with M v ≈ -21.6 and a tidally disrupted satellite galaxy with M v PS -17.7 at a photometric redshift of z ≈ 0.08. This redshift is consistent with the spectroscopic redshift of 0.079 for the giant elliptical galaxy obtained from the Sloan Digital Sky Survey (SDSS) archive. The luminosity masses of the two galaxies are 3.7 × 10 12 and 3.7 × 10 9 M ⊙, respectively. The distance between the two galaxies is greater than 100 kpc. The two tidal tails emanating from the satellite galaxy extend over 150 kpc. This system would be the second well-defined galaxy threshing system found so far.

AB - We report on the discovery of a new potential galaxy threshing system in the COSMOS 2 square degree field using the prime-focus camera, Suprime-Cam, on the 8.2 m Subaru Telescope. This system consists of a giant elliptical galaxy with M v ≈ -21.6 and a tidally disrupted satellite galaxy with M v PS -17.7 at a photometric redshift of z ≈ 0.08. This redshift is consistent with the spectroscopic redshift of 0.079 for the giant elliptical galaxy obtained from the Sloan Digital Sky Survey (SDSS) archive. The luminosity masses of the two galaxies are 3.7 × 10 12 and 3.7 × 10 9 M ⊙, respectively. The distance between the two galaxies is greater than 100 kpc. The two tidal tails emanating from the satellite galaxy extend over 150 kpc. This system would be the second well-defined galaxy threshing system found so far.

KW - Galaxies: evolution

KW - Galaxies: interactions

UR - https://www.scopus.com/pages/publications/35348824815

U2 - 10.1086/516581

DO - 10.1086/516581

M3 - Article

AN - SCOPUS:35348824815

SN - 0067-0049

VL - 172

SP - 511

EP - 517

JO - Astrophysical Journal, Supplement Series

JF - Astrophysical Journal, Supplement Series

IS - 1

ER -

A potential galaxy threshing system in the COSMOS field

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Keywords

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