V838 monocerotis: A geometric distance from hubble space telescope polarimetric imaging of its light echo

William B. Sparks, Howard E. Bond, Misty Cracraft, Zolt Levay, Lisa A. Crause, Michael A. Dopita, Arne A. Henden, Ulisse Munari, Nino Panagia, Sumner G. Starrfield, Ben E. Sugerman, R. Mark Wagner, Richard L. White

Research output: Contribution to journalArticle

45 Citations (Scopus)

Abstract

Following the outburst of the unusual variable star V838 Monocerotis in 2002, a spectacular light echo appeared. A light echo provides the possibility of direct geometric distance determination, because it should contain a ring of highly linearly polarized light at a linear radius of ct, where t is the time since the outburst. We present imaging polarimetry of the V838 Mon light echo, obtained in 2002 and 2005 with the Advanced Camera for Surveys on board the Hubble Space Telescope, which confirms the presence of the highly polarized ring. Based on detailed modeling that takes into account the outburst light curve, the paraboloidal echo geometry, and the physics of dust scattering and polarization, we find a distance of 6.1 0.6 kpc. The error is dominated by the systematic uncertainty in the scattering angle of maximum linear polarization, taken to be θmax = 90° 5°. The polarimetric distance agrees remarkably well with a distance of 6.2 1.2 kpc obtained from the entirely independent method of main-sequence fitting to a sparse star cluster associated with V838 Mon. At this distance, V838 Mon at maximum light had MV ≃ -9.8, making it temporarily one of the most luminous stars in the Local Group. Our validation of the polarimetric method offers promise for measurement of extragalactic distances using supernova light echoes.

Original languageEnglish (US)
Pages (from-to)605-617
Number of pages13
JournalAstronomical Journal
Volume135
Issue number2
DOIs
StatePublished - Feb 1 2008

Fingerprint

Hubble Space Telescope
echoes
outburst
polarization
scattering
variable stars
rings
polarimetry
star clusters
linear polarization
polarized light
light curve
supernovae
dust
cameras
physics
stars
radii
geometry
modeling

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Sparks, William B. ; Bond, Howard E. ; Cracraft, Misty ; Levay, Zolt ; Crause, Lisa A. ; Dopita, Michael A. ; Henden, Arne A. ; Munari, Ulisse ; Panagia, Nino ; Starrfield, Sumner G. ; Sugerman, Ben E. ; Wagner, R. Mark ; White, Richard L. / V838 monocerotis : A geometric distance from hubble space telescope polarimetric imaging of its light echo. In: Astronomical Journal. 2008 ; Vol. 135, No. 2. pp. 605-617.
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abstract = "Following the outburst of the unusual variable star V838 Monocerotis in 2002, a spectacular light echo appeared. A light echo provides the possibility of direct geometric distance determination, because it should contain a ring of highly linearly polarized light at a linear radius of ct, where t is the time since the outburst. We present imaging polarimetry of the V838 Mon light echo, obtained in 2002 and 2005 with the Advanced Camera for Surveys on board the Hubble Space Telescope, which confirms the presence of the highly polarized ring. Based on detailed modeling that takes into account the outburst light curve, the paraboloidal echo geometry, and the physics of dust scattering and polarization, we find a distance of 6.1 0.6 kpc. The error is dominated by the systematic uncertainty in the scattering angle of maximum linear polarization, taken to be θmax = 90° 5°. The polarimetric distance agrees remarkably well with a distance of 6.2 1.2 kpc obtained from the entirely independent method of main-sequence fitting to a sparse star cluster associated with V838 Mon. At this distance, V838 Mon at maximum light had MV ≃ -9.8, making it temporarily one of the most luminous stars in the Local Group. Our validation of the polarimetric method offers promise for measurement of extragalactic distances using supernova light echoes.",
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Sparks, WB, Bond, HE, Cracraft, M, Levay, Z, Crause, LA, Dopita, MA, Henden, AA, Munari, U, Panagia, N, Starrfield, SG, Sugerman, BE, Wagner, RM & White, RL 2008, 'V838 monocerotis: A geometric distance from hubble space telescope polarimetric imaging of its light echo', Astronomical Journal, vol. 135, no. 2, pp. 605-617. https://doi.org/10.1088/0004-6256/135/2/605

V838 monocerotis : A geometric distance from hubble space telescope polarimetric imaging of its light echo. / Sparks, William B.; Bond, Howard E.; Cracraft, Misty; Levay, Zolt; Crause, Lisa A.; Dopita, Michael A.; Henden, Arne A.; Munari, Ulisse; Panagia, Nino; Starrfield, Sumner G.; Sugerman, Ben E.; Wagner, R. Mark; White, Richard L.

In: Astronomical Journal, Vol. 135, No. 2, 01.02.2008, p. 605-617.

Research output: Contribution to journalArticle

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T2 - A geometric distance from hubble space telescope polarimetric imaging of its light echo

AU - Sparks, William B.

AU - Bond, Howard E.

AU - Cracraft, Misty

AU - Levay, Zolt

AU - Crause, Lisa A.

AU - Dopita, Michael A.

AU - Henden, Arne A.

AU - Munari, Ulisse

AU - Panagia, Nino

AU - Starrfield, Sumner G.

AU - Sugerman, Ben E.

AU - Wagner, R. Mark

AU - White, Richard L.

PY - 2008/2/1

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N2 - Following the outburst of the unusual variable star V838 Monocerotis in 2002, a spectacular light echo appeared. A light echo provides the possibility of direct geometric distance determination, because it should contain a ring of highly linearly polarized light at a linear radius of ct, where t is the time since the outburst. We present imaging polarimetry of the V838 Mon light echo, obtained in 2002 and 2005 with the Advanced Camera for Surveys on board the Hubble Space Telescope, which confirms the presence of the highly polarized ring. Based on detailed modeling that takes into account the outburst light curve, the paraboloidal echo geometry, and the physics of dust scattering and polarization, we find a distance of 6.1 0.6 kpc. The error is dominated by the systematic uncertainty in the scattering angle of maximum linear polarization, taken to be θmax = 90° 5°. The polarimetric distance agrees remarkably well with a distance of 6.2 1.2 kpc obtained from the entirely independent method of main-sequence fitting to a sparse star cluster associated with V838 Mon. At this distance, V838 Mon at maximum light had MV ≃ -9.8, making it temporarily one of the most luminous stars in the Local Group. Our validation of the polarimetric method offers promise for measurement of extragalactic distances using supernova light echoes.

AB - Following the outburst of the unusual variable star V838 Monocerotis in 2002, a spectacular light echo appeared. A light echo provides the possibility of direct geometric distance determination, because it should contain a ring of highly linearly polarized light at a linear radius of ct, where t is the time since the outburst. We present imaging polarimetry of the V838 Mon light echo, obtained in 2002 and 2005 with the Advanced Camera for Surveys on board the Hubble Space Telescope, which confirms the presence of the highly polarized ring. Based on detailed modeling that takes into account the outburst light curve, the paraboloidal echo geometry, and the physics of dust scattering and polarization, we find a distance of 6.1 0.6 kpc. The error is dominated by the systematic uncertainty in the scattering angle of maximum linear polarization, taken to be θmax = 90° 5°. The polarimetric distance agrees remarkably well with a distance of 6.2 1.2 kpc obtained from the entirely independent method of main-sequence fitting to a sparse star cluster associated with V838 Mon. At this distance, V838 Mon at maximum light had MV ≃ -9.8, making it temporarily one of the most luminous stars in the Local Group. Our validation of the polarimetric method offers promise for measurement of extragalactic distances using supernova light echoes.

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