Supernova remnants, planetary nebulae and the distance to NGC 4214

Michael A. Dopita; Daniela Calzetti; Jesús Maíz Apellániz; William P. Blair; Knox S. Long; Max Mutchler; Bradley C. Whitmore; Howard E. Bond; John MacKenty; Bruce Balick; Marcella Carollo; Michael Disney; Jay A. Frogel; Robert O'Connell; Donald Hall; Jon A. Holtzman; Randy A. Kimble; Patrick McCarthy; Francesco Paresce; Abhijit Saha; Alistair R. Walker; Joe Silk; Marco Sirianni; John Trauger; Rogier Windhorst; Erick Young

doi:10.1007/s10509-010-0376-0

Supernova remnants, planetary nebulae and the distance to NGC 4214

Michael A. Dopita, Daniela Calzetti, Jesús Maíz Apellániz, William P. Blair, Knox S. Long, Max Mutchler, Bradley C. Whitmore, Howard E. Bond, John MacKenty, Bruce Balick, Marcella Carollo, Michael Disney, Jay A. Frogel, Robert O'Connell, Donald Hall, Jon A. Holtzman, Randy A. Kimble, Patrick McCarthy, Francesco Paresce, Abhijit SahaAlistair R. Walker, Joe Silk, Marco Sirianni, John Trauger, Rogier Windhorst, Erick Young

Astronomy & Astrophysics

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

17 Scopus citations

Abstract

We present narrow band, continuum subtracted Hα, [S II], Hβ, [O III] and [O II] data taken with the Wide Field Camera 3 on the Hubble Space Telescope in the nearby dwarf starburst galaxy NGC 4214. From these images, we identify seventeen new planetary nebula candidates, and seven supernova remnant candidates. We use the observed emission line luminosity function of the planetary nebulae to establish a new velocity-independent distance to NGC 4214. We conclude that the PNLF technique gives a reddening independent distance to NGC 4214 of 3.19±0.36 Mpc, and that our current best-estimate of the distance to this galaxy ids 2.98±0.13 Mpc.

Original language	English (US)
Pages (from-to)	123-131
Number of pages	9
Journal	Astrophysics and Space Science
Volume	330
Issue number	1
DOIs	https://doi.org/10.1007/s10509-010-0376-0
State	Published - Jan 1 2010

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1007/s10509-010-0376-0

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Dopita, M. A., Calzetti, D., Maíz Apellániz, J., Blair, W. P., Long, K. S., Mutchler, M., Whitmore, B. C., Bond, H. E., MacKenty, J., Balick, B., Carollo, M., Disney, M., Frogel, J. A., O'Connell, R., Hall, D., Holtzman, J. A., Kimble, R. A., McCarthy, P., Paresce, F., ... Young, E. (2010). Supernova remnants, planetary nebulae and the distance to NGC 4214. Astrophysics and Space Science, 330(1), 123-131. https://doi.org/10.1007/s10509-010-0376-0

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title = "Supernova remnants, planetary nebulae and the distance to NGC 4214",

abstract = "We present narrow band, continuum subtracted Hα, [S II], Hβ, [O III] and [O II] data taken with the Wide Field Camera 3 on the Hubble Space Telescope in the nearby dwarf starburst galaxy NGC 4214. From these images, we identify seventeen new planetary nebula candidates, and seven supernova remnant candidates. We use the observed emission line luminosity function of the planetary nebulae to establish a new velocity-independent distance to NGC 4214. We conclude that the PNLF technique gives a reddening independent distance to NGC 4214 of 3.19±0.36 Mpc, and that our current best-estimate of the distance to this galaxy ids 2.98±0.13 Mpc.",

author = "Dopita, {Michael A.} and Daniela Calzetti and Jes{\'u}s Ma{\'i}z Apell{\'a}niz and Blair, {William P.} and Long, {Knox S.} and Max Mutchler and Whitmore, {Bradley C.} and Bond, {Howard E.} and John MacKenty and Bruce Balick and Marcella Carollo and Michael Disney and Frogel, {Jay A.} and Robert O'Connell and Donald Hall and Holtzman, {Jon A.} and Kimble, {Randy A.} and Patrick McCarthy and Francesco Paresce and Abhijit Saha and Walker, {Alistair R.} and Joe Silk and Marco Sirianni and John Trauger and Rogier Windhorst and Erick Young",

year = "2010",

month = jan,

day = "1",

doi = "10.1007/s10509-010-0376-0",

language = "English (US)",

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Dopita, MA, Calzetti, D, Maíz Apellániz, J, Blair, WP, Long, KS, Mutchler, M, Whitmore, BC, Bond, HE, MacKenty, J, Balick, B, Carollo, M, Disney, M, Frogel, JA, O'Connell, R, Hall, D, Holtzman, JA, Kimble, RA, McCarthy, P, Paresce, F, Saha, A, Walker, AR, Silk, J, Sirianni, M, Trauger, J, Windhorst, R & Young, E 2010, 'Supernova remnants, planetary nebulae and the distance to NGC 4214', Astrophysics and Space Science, vol. 330, no. 1, pp. 123-131. https://doi.org/10.1007/s10509-010-0376-0

TY - JOUR

T1 - Supernova remnants, planetary nebulae and the distance to NGC 4214

AU - Dopita, Michael A.

AU - Calzetti, Daniela

AU - Maíz Apellániz, Jesús

AU - Blair, William P.

AU - Long, Knox S.

AU - Mutchler, Max

AU - Whitmore, Bradley C.

AU - Bond, Howard E.

AU - MacKenty, John

AU - Balick, Bruce

AU - Carollo, Marcella

AU - Disney, Michael

AU - Frogel, Jay A.

AU - O'Connell, Robert

AU - Hall, Donald

AU - Holtzman, Jon A.

AU - Kimble, Randy A.

AU - McCarthy, Patrick

AU - Paresce, Francesco

AU - Saha, Abhijit

AU - Walker, Alistair R.

AU - Silk, Joe

AU - Sirianni, Marco

AU - Trauger, John

AU - Windhorst, Rogier

AU - Young, Erick

PY - 2010/1/1

Y1 - 2010/1/1

N2 - We present narrow band, continuum subtracted Hα, [S II], Hβ, [O III] and [O II] data taken with the Wide Field Camera 3 on the Hubble Space Telescope in the nearby dwarf starburst galaxy NGC 4214. From these images, we identify seventeen new planetary nebula candidates, and seven supernova remnant candidates. We use the observed emission line luminosity function of the planetary nebulae to establish a new velocity-independent distance to NGC 4214. We conclude that the PNLF technique gives a reddening independent distance to NGC 4214 of 3.19±0.36 Mpc, and that our current best-estimate of the distance to this galaxy ids 2.98±0.13 Mpc.

AB - We present narrow band, continuum subtracted Hα, [S II], Hβ, [O III] and [O II] data taken with the Wide Field Camera 3 on the Hubble Space Telescope in the nearby dwarf starburst galaxy NGC 4214. From these images, we identify seventeen new planetary nebula candidates, and seven supernova remnant candidates. We use the observed emission line luminosity function of the planetary nebulae to establish a new velocity-independent distance to NGC 4214. We conclude that the PNLF technique gives a reddening independent distance to NGC 4214 of 3.19±0.36 Mpc, and that our current best-estimate of the distance to this galaxy ids 2.98±0.13 Mpc.

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U2 - 10.1007/s10509-010-0376-0

DO - 10.1007/s10509-010-0376-0

M3 - Article

SN - 0004-640X

VL - 330

SP - 123

EP - 131

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

IS - 1

ER -

Supernova remnants, planetary nebulae and the distance to NGC 4214

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