Two serendipitous low-mass LMC clusters discovered with HST

Basílio X. Santiago, Rebecca A.W. Elson, Steinn Sigurdsson, Gerard F. Gilmore

Research output: Contribution to journalArticle

4 Citations (Scopus)

Abstract

We present V and I photometry of two open clusters in the LMC down to V∼26. The clusters were imaged with the Wide Field and Planetary Camera 2 (WFPC2) on board the Hubble Space Telescope (HST), as part of the Medium Deep Survey Key Project. Both are low-luminosity (Mv ∼ - 3.5), low-mass (M ∼ 103 M) systems. The chance discovery of these two clusters in two parallel WFPC2 fields suggests a significant incompleteness in the LMC cluster census near the bar. One of the clusters is roughly elliptical and compact, with a steep light profile, a central surface brightness μv(0)∼20.2 mag arcsec-2, a half-light radius rhl∼0.9 pc (total visual major diameter D ∼ 3 pc) and an estimated mass M ∼ 1500 M. From the colour-magnitude diagram and isochrone fits we estimate its age as τ ∼(2-5) × 108 yr. Its mass function has a fitted slope of Γ = Δ log φ(M )/ΔlogM= - 1.8±0.7 in the range probed (0.9≲M/M≲4.5). The other cluster is more irregular and sparse, having shallower density and surface brightness profiles. We obtain Γ= -1.2±0.4, and estimate its mass as M∼400 M. A derived upper limit for its age is τ≲5 × 108 yr. Both clusters have mass functions with slopes similar to that of R136, a massive LMC cluster, for which HST results indicate Γ ∼ - 1.2. They also seem to be relaxed in their cores and well contained in their tidal radii.

Original languageEnglish (US)
Pages (from-to)860-868
Number of pages9
JournalMonthly Notices of the Royal Astronomical Society
Volume295
Issue number4
DOIs
StatePublished - Apr 21 1998

Fingerprint

Hubble Space Telescope
brightness
cameras
slopes
census
radii
color-magnitude diagram
open clusters
diagram
estimates
profiles
photometry
luminosity

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Santiago, Basílio X. ; Elson, Rebecca A.W. ; Sigurdsson, Steinn ; Gilmore, Gerard F. / Two serendipitous low-mass LMC clusters discovered with HST. In: Monthly Notices of the Royal Astronomical Society. 1998 ; Vol. 295, No. 4. pp. 860-868.
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abstract = "We present V and I photometry of two open clusters in the LMC down to V∼26. The clusters were imaged with the Wide Field and Planetary Camera 2 (WFPC2) on board the Hubble Space Telescope (HST), as part of the Medium Deep Survey Key Project. Both are low-luminosity (Mv ∼ - 3.5), low-mass (M ∼ 103 M⊙) systems. The chance discovery of these two clusters in two parallel WFPC2 fields suggests a significant incompleteness in the LMC cluster census near the bar. One of the clusters is roughly elliptical and compact, with a steep light profile, a central surface brightness μv(0)∼20.2 mag arcsec-2, a half-light radius rhl∼0.9 pc (total visual major diameter D ∼ 3 pc) and an estimated mass M ∼ 1500 M⊙. From the colour-magnitude diagram and isochrone fits we estimate its age as τ ∼(2-5) × 108 yr. Its mass function has a fitted slope of Γ = Δ log φ(M )/ΔlogM= - 1.8±0.7 in the range probed (0.9≲M/M⊙≲4.5). The other cluster is more irregular and sparse, having shallower density and surface brightness profiles. We obtain Γ= -1.2±0.4, and estimate its mass as M∼400 M⊙. A derived upper limit for its age is τ≲5 × 108 yr. Both clusters have mass functions with slopes similar to that of R136, a massive LMC cluster, for which HST results indicate Γ ∼ - 1.2. They also seem to be relaxed in their cores and well contained in their tidal radii.",
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Two serendipitous low-mass LMC clusters discovered with HST. / Santiago, Basílio X.; Elson, Rebecca A.W.; Sigurdsson, Steinn; Gilmore, Gerard F.

In: Monthly Notices of the Royal Astronomical Society, Vol. 295, No. 4, 21.04.1998, p. 860-868.

Research output: Contribution to journalArticle

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T1 - Two serendipitous low-mass LMC clusters discovered with HST

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N2 - We present V and I photometry of two open clusters in the LMC down to V∼26. The clusters were imaged with the Wide Field and Planetary Camera 2 (WFPC2) on board the Hubble Space Telescope (HST), as part of the Medium Deep Survey Key Project. Both are low-luminosity (Mv ∼ - 3.5), low-mass (M ∼ 103 M⊙) systems. The chance discovery of these two clusters in two parallel WFPC2 fields suggests a significant incompleteness in the LMC cluster census near the bar. One of the clusters is roughly elliptical and compact, with a steep light profile, a central surface brightness μv(0)∼20.2 mag arcsec-2, a half-light radius rhl∼0.9 pc (total visual major diameter D ∼ 3 pc) and an estimated mass M ∼ 1500 M⊙. From the colour-magnitude diagram and isochrone fits we estimate its age as τ ∼(2-5) × 108 yr. Its mass function has a fitted slope of Γ = Δ log φ(M )/ΔlogM= - 1.8±0.7 in the range probed (0.9≲M/M⊙≲4.5). The other cluster is more irregular and sparse, having shallower density and surface brightness profiles. We obtain Γ= -1.2±0.4, and estimate its mass as M∼400 M⊙. A derived upper limit for its age is τ≲5 × 108 yr. Both clusters have mass functions with slopes similar to that of R136, a massive LMC cluster, for which HST results indicate Γ ∼ - 1.2. They also seem to be relaxed in their cores and well contained in their tidal radii.

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