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Distance scale calibration from kinematic analysis of an ensemble of the galactic planetary nebulae. / Akimkin, V.V.; Nikiforov, I.I.; Kholtygin, A.F.

In: Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society, Vol. 27, No. 2, 2012, p. 365-368.

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Akimkin VV, Nikiforov II, Kholtygin AF. Distance scale calibration from kinematic analysis of an ensemble of the galactic planetary nebulae. Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society. 2012;27(2):365-368.

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Akimkin, V.V. ; Nikiforov, I.I. ; Kholtygin, A.F. / Distance scale calibration from kinematic analysis of an ensemble of the galactic planetary nebulae. In: Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society. 2012 ; Vol. 27, No. 2. pp. 365-368.

BibTeX

@article{b46b83e243c84c0380d3968538a99f85,
title = "Distance scale calibration from kinematic analysis of an ensemble of the galactic planetary nebulae",
abstract = "We study the kinematics of ensembles of planetary nebulae (PNe) of the Galactic disk using the PN distance catalogues by Acker (1978), Cahn et al. (1992), and Phillips (2004). Formal values for the Galactic center distance, $R_0$, derived from kinematic analysis of the PNe with distance scales accepted in the catalogues were found to be low, from 5 to 7 kpc. To correct these underestimated distance scales we renormalized the PN distances using the ratios of formal $R_0$ values to a best modern value of $R_0 =7.9$ kpc deduced from many original estimates. A new catalogue of distances for the Galactic disk's PNe was created by averaging the kinematically corrected distances to PNe obtained for the catalogues mentioned above. New distances for Peimbert's types I and II PNe are in a good agreement with distances by Stanghellini et al.\ (2008). Our new catalog of PNe distances was used to recalibrate statistical distance scales for all types of PNe.",
keywords = "Galaxy, Planetary nebulae, Kinematics, Distance scales, Galactic center distance",
author = "V.V. Akimkin and I.I. Nikiforov and A.F. Kholtygin",
year = "2012",
language = "English",
volume = "27",
pages = "365--368",
journal = "Astronomical and Astrophysical Transactions",
issn = "1055-6796",
publisher = "Cambridge Scientific Publishers",
number = "2",

}

RIS

TY - JOUR

T1 - Distance scale calibration from kinematic analysis of an ensemble of the galactic planetary nebulae

AU - Akimkin, V.V.

AU - Nikiforov, I.I.

AU - Kholtygin, A.F.

PY - 2012

Y1 - 2012

N2 - We study the kinematics of ensembles of planetary nebulae (PNe) of the Galactic disk using the PN distance catalogues by Acker (1978), Cahn et al. (1992), and Phillips (2004). Formal values for the Galactic center distance, $R_0$, derived from kinematic analysis of the PNe with distance scales accepted in the catalogues were found to be low, from 5 to 7 kpc. To correct these underestimated distance scales we renormalized the PN distances using the ratios of formal $R_0$ values to a best modern value of $R_0 =7.9$ kpc deduced from many original estimates. A new catalogue of distances for the Galactic disk's PNe was created by averaging the kinematically corrected distances to PNe obtained for the catalogues mentioned above. New distances for Peimbert's types I and II PNe are in a good agreement with distances by Stanghellini et al.\ (2008). Our new catalog of PNe distances was used to recalibrate statistical distance scales for all types of PNe.

AB - We study the kinematics of ensembles of planetary nebulae (PNe) of the Galactic disk using the PN distance catalogues by Acker (1978), Cahn et al. (1992), and Phillips (2004). Formal values for the Galactic center distance, $R_0$, derived from kinematic analysis of the PNe with distance scales accepted in the catalogues were found to be low, from 5 to 7 kpc. To correct these underestimated distance scales we renormalized the PN distances using the ratios of formal $R_0$ values to a best modern value of $R_0 =7.9$ kpc deduced from many original estimates. A new catalogue of distances for the Galactic disk's PNe was created by averaging the kinematically corrected distances to PNe obtained for the catalogues mentioned above. New distances for Peimbert's types I and II PNe are in a good agreement with distances by Stanghellini et al.\ (2008). Our new catalog of PNe distances was used to recalibrate statistical distance scales for all types of PNe.

KW - Galaxy

KW - Planetary nebulae

KW - Kinematics

KW - Distance scales

KW - Galactic center distance

M3 - Article

VL - 27

SP - 365

EP - 368

JO - Astronomical and Astrophysical Transactions

JF - Astronomical and Astrophysical Transactions

SN - 1055-6796

IS - 2

ER -

ID: 5335759