Home > Research > Publications & Outputs > Another look at the size of the low-surface bri...

Associated organisational unit

Electronic data

  • 1610.07831

    Rights statement: This is the peer reviewed version of the following article: Koch A, Black CS, Rich RM, Longstaff FA, Collins MLM, Janz J. Another look at the size of the low-surface-brightness galaxy VCC 1661 in the Virgo Cluster. Astron. Nachr. / AN. 2017;338:503–509. https://doi.org/10.1002/asna.201613274 which has been published in final form at http://onlinelibrary.wiley.com/doi/10.1002/asna.201613274/abstract This article may be used for non-commercial purposes in accordance With Wiley Terms and Conditions for self-archiving.

    Accepted author manuscript, 1.55 MB, PDF document

    Available under license: CC BY-NC: Creative Commons Attribution-NonCommercial 4.0 International License

Links

Text available via DOI:

View graph of relations

Another look at the size of the low-surface brightness galaxy VCC 1661 in the Virgo Cluster

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Published

Standard

Another look at the size of the low-surface brightness galaxy VCC 1661 in the Virgo Cluster. / Koch, Andreas; Black, Christine S.; Rich, R. Michael et al.
In: Astronomical Notes / Astronomische Nachrichten, Vol. 338, No. 4, 05.2017, p. 503-509.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Koch, A, Black, CS, Rich, RM, Longstaff, FA, Collins, MLM & Janz, J 2017, 'Another look at the size of the low-surface brightness galaxy VCC 1661 in the Virgo Cluster', Astronomical Notes / Astronomische Nachrichten, vol. 338, no. 4, pp. 503-509. https://doi.org/10.1002/asna.201613274

APA

Koch, A., Black, C. S., Rich, R. M., Longstaff, F. A., Collins, M. L. M., & Janz, J. (2017). Another look at the size of the low-surface brightness galaxy VCC 1661 in the Virgo Cluster. Astronomical Notes / Astronomische Nachrichten, 338(4), 503-509. https://doi.org/10.1002/asna.201613274

Vancouver

Koch A, Black CS, Rich RM, Longstaff FA, Collins MLM, Janz J. Another look at the size of the low-surface brightness galaxy VCC 1661 in the Virgo Cluster. Astronomical Notes / Astronomische Nachrichten. 2017 May;338(4):503-509. Epub 2017 Feb 15. doi: 10.1002/asna.201613274

Author

Koch, Andreas ; Black, Christine S. ; Rich, R. Michael et al. / Another look at the size of the low-surface brightness galaxy VCC 1661 in the Virgo Cluster. In: Astronomical Notes / Astronomische Nachrichten. 2017 ; Vol. 338, No. 4. pp. 503-509.

Bibtex

@article{51771cd8746e4a7abb2470e314e1971e,
title = "Another look at the size of the low-surface brightness galaxy VCC 1661 in the Virgo Cluster",
abstract = "We present new wide-field images of the low-surface brightness Virgo Cluster dwarf galaxy VCC 1661. The extant literature lists a broad range of radii for this object, covering a factor of more than four, depending on the filters used and the details of the analyses. While some studies find a radius typical of other Virgo dwarfs and note the normality of this object, any larger spatial extent, taken at face value, would render this galaxy the largest dwarf in the Virgo Cluster samples.Confirmation of a large extent of dwarf galaxies has often led to the discovery of tidal tails and would then, also in VCC 1661, indicate a severe state of tidal disruption. Given the importance of galactic sizes for assessing tidal interactions of the satellites with their hosts, we thus combine our surface brightness profile with data from the literature to investigate further the nature of this galaxy. However, our new characteristic radius for VCC 1661 of re = 24.1′′ ± 7.7 ′′ and thepreviously noted smooth appearance of its isophotes are fully consistent with the remainder of the ACSVCS dwarf galaxy population without any need to invoke tidal perturbations.",
author = "Andreas Koch and Black, {Christine S.} and Rich, {R. Michael} and Longstaff, {Francis A.} and Collins, {Michelle L. M.} and Joachim Janz",
note = "This is the peer reviewed version of the following article: Koch A, Black CS, Rich RM, Longstaff FA, Collins MLM, Janz J. Another look at the size of the low-surface-brightness galaxy VCC 1661 in the Virgo Cluster. Astron. Nachr. / AN. 2017;338:503–509. https://doi.org/10.1002/asna.201613274 which has been published in final form at http://onlinelibrary.wiley.com/doi/10.1002/asna.201613274/abstract This article may be used for non-commercial purposes in accordance With Wiley Terms and Conditions for self-archiving.",
year = "2017",
month = may,
doi = "10.1002/asna.201613274",
language = "English",
volume = "338",
pages = "503--509",
journal = "Astronomical Notes / Astronomische Nachrichten",
issn = "0004-6337",
publisher = "Wiley",
number = "4",

}

RIS

TY - JOUR

T1 - Another look at the size of the low-surface brightness galaxy VCC 1661 in the Virgo Cluster

AU - Koch, Andreas

AU - Black, Christine S.

AU - Rich, R. Michael

AU - Longstaff, Francis A.

AU - Collins, Michelle L. M.

AU - Janz, Joachim

N1 - This is the peer reviewed version of the following article: Koch A, Black CS, Rich RM, Longstaff FA, Collins MLM, Janz J. Another look at the size of the low-surface-brightness galaxy VCC 1661 in the Virgo Cluster. Astron. Nachr. / AN. 2017;338:503–509. https://doi.org/10.1002/asna.201613274 which has been published in final form at http://onlinelibrary.wiley.com/doi/10.1002/asna.201613274/abstract This article may be used for non-commercial purposes in accordance With Wiley Terms and Conditions for self-archiving.

PY - 2017/5

Y1 - 2017/5

N2 - We present new wide-field images of the low-surface brightness Virgo Cluster dwarf galaxy VCC 1661. The extant literature lists a broad range of radii for this object, covering a factor of more than four, depending on the filters used and the details of the analyses. While some studies find a radius typical of other Virgo dwarfs and note the normality of this object, any larger spatial extent, taken at face value, would render this galaxy the largest dwarf in the Virgo Cluster samples.Confirmation of a large extent of dwarf galaxies has often led to the discovery of tidal tails and would then, also in VCC 1661, indicate a severe state of tidal disruption. Given the importance of galactic sizes for assessing tidal interactions of the satellites with their hosts, we thus combine our surface brightness profile with data from the literature to investigate further the nature of this galaxy. However, our new characteristic radius for VCC 1661 of re = 24.1′′ ± 7.7 ′′ and thepreviously noted smooth appearance of its isophotes are fully consistent with the remainder of the ACSVCS dwarf galaxy population without any need to invoke tidal perturbations.

AB - We present new wide-field images of the low-surface brightness Virgo Cluster dwarf galaxy VCC 1661. The extant literature lists a broad range of radii for this object, covering a factor of more than four, depending on the filters used and the details of the analyses. While some studies find a radius typical of other Virgo dwarfs and note the normality of this object, any larger spatial extent, taken at face value, would render this galaxy the largest dwarf in the Virgo Cluster samples.Confirmation of a large extent of dwarf galaxies has often led to the discovery of tidal tails and would then, also in VCC 1661, indicate a severe state of tidal disruption. Given the importance of galactic sizes for assessing tidal interactions of the satellites with their hosts, we thus combine our surface brightness profile with data from the literature to investigate further the nature of this galaxy. However, our new characteristic radius for VCC 1661 of re = 24.1′′ ± 7.7 ′′ and thepreviously noted smooth appearance of its isophotes are fully consistent with the remainder of the ACSVCS dwarf galaxy population without any need to invoke tidal perturbations.

U2 - 10.1002/asna.201613274

DO - 10.1002/asna.201613274

M3 - Journal article

VL - 338

SP - 503

EP - 509

JO - Astronomical Notes / Astronomische Nachrichten

JF - Astronomical Notes / Astronomische Nachrichten

SN - 0004-6337

IS - 4

ER -