IPHAS extinction distances to planetary nebulae

C. Giammanco; S. E. Sale; R. L M Corradi; M. J. Barlow; K. Viironen; L. Sabin; M. Santander-García; D. J. Frew; R. Greimel; B. Miszalski; S. Phillipps; A. A. Zijlstra; A. Mampaso; J. E. Drew; Q. A. Parker; R. Napiwotzki

doi:10.1051/0004-6361/201014464

IPHAS extinction distances to planetary nebulae

C. Giammanco^*, S. E. Sale, R. L M Corradi, M. J. Barlow, K. Viironen, L. Sabin, M. Santander-García, D. J. Frew, R. Greimel, B. Miszalski, S. Phillipps, A. A. Zijlstra, A. Mampaso, J. E. Drew, Q. A. Parker, R. Napiwotzki

^*Corresponding author for this work

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

38 Citations (Scopus)

Abstract

Aims. The determination of reliable distances to planetary nebulae (PNe) is a major difficulty in the study of this class of objects in the Galaxy. The availability of new photometric surveys such as IPHAS (the INT/WFC photometric H_α survey of the northern Galactic plane) covering large portions of the sky provide an opportunity to apply the so-called extinction method to determine the distances of a large number of objects. Methods. The technique is applied to a sample of 137 PNe located between -5 and 5 degrees in Galactic latitude, and between 29.52 and 215.49 degrees in longitude. The characteristics of the distance-extinction method and the main sources of errors are carefully discussed. Results. The data on the extinction of the PNe available in the literature, complemented by new observations, allow us to determine extinction distances for 70 PNe. A comparison with statistical distance scales from different authors is presented.

Original language	English
Article number	A58
Pages (from-to)	1-11
Number of pages	11
Journal	Astronomy and Astrophysics
Volume	525
DOIs	https://doi.org/10.1051/0004-6361/201014464
Publication status	Published - Jan 2011

Keywords

catalogs
planetary nebulae: general

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10.1051/0004-6361/201014464

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Giammanco, C., Sale, S. E., Corradi, R. L. M., Barlow, M. J., Viironen, K., Sabin, L., Santander-García, M., Frew, D. J., Greimel, R., Miszalski, B., Phillipps, S., Zijlstra, A. A., Mampaso, A., Drew, J. E., Parker, Q. A., & Napiwotzki, R. (2011). IPHAS extinction distances to planetary nebulae. Astronomy and Astrophysics, 525, 1-11. Article A58. https://doi.org/10.1051/0004-6361/201014464

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abstract = "Aims. The determination of reliable distances to planetary nebulae (PNe) is a major difficulty in the study of this class of objects in the Galaxy. The availability of new photometric surveys such as IPHAS (the INT/WFC photometric Hα survey of the northern Galactic plane) covering large portions of the sky provide an opportunity to apply the so-called extinction method to determine the distances of a large number of objects. Methods. The technique is applied to a sample of 137 PNe located between -5 and 5 degrees in Galactic latitude, and between 29.52 and 215.49 degrees in longitude. The characteristics of the distance-extinction method and the main sources of errors are carefully discussed. Results. The data on the extinction of the PNe available in the literature, complemented by new observations, allow us to determine extinction distances for 70 PNe. A comparison with statistical distance scales from different authors is presented.",

keywords = "catalogs, planetary nebulae: general",

author = "C. Giammanco and Sale, {S. E.} and Corradi, {R. L M} and Barlow, {M. J.} and K. Viironen and L. Sabin and M. Santander-Garc{\'i}a and Frew, {D. J.} and R. Greimel and B. Miszalski and S. Phillipps and Zijlstra, {A. A.} and A. Mampaso and Drew, {J. E.} and Parker, {Q. A.} and R. Napiwotzki",

year = "2011",

month = jan,

doi = "10.1051/0004-6361/201014464",

language = "English",

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AU - Giammanco, C.

AU - Sale, S. E.

AU - Corradi, R. L M

AU - Barlow, M. J.

AU - Viironen, K.

AU - Sabin, L.

AU - Santander-García, M.

AU - Frew, D. J.

AU - Greimel, R.

AU - Miszalski, B.

AU - Phillipps, S.

AU - Zijlstra, A. A.

AU - Mampaso, A.

AU - Drew, J. E.

AU - Parker, Q. A.

AU - Napiwotzki, R.

PY - 2011/1

Y1 - 2011/1

N2 - Aims. The determination of reliable distances to planetary nebulae (PNe) is a major difficulty in the study of this class of objects in the Galaxy. The availability of new photometric surveys such as IPHAS (the INT/WFC photometric Hα survey of the northern Galactic plane) covering large portions of the sky provide an opportunity to apply the so-called extinction method to determine the distances of a large number of objects. Methods. The technique is applied to a sample of 137 PNe located between -5 and 5 degrees in Galactic latitude, and between 29.52 and 215.49 degrees in longitude. The characteristics of the distance-extinction method and the main sources of errors are carefully discussed. Results. The data on the extinction of the PNe available in the literature, complemented by new observations, allow us to determine extinction distances for 70 PNe. A comparison with statistical distance scales from different authors is presented.

AB - Aims. The determination of reliable distances to planetary nebulae (PNe) is a major difficulty in the study of this class of objects in the Galaxy. The availability of new photometric surveys such as IPHAS (the INT/WFC photometric Hα survey of the northern Galactic plane) covering large portions of the sky provide an opportunity to apply the so-called extinction method to determine the distances of a large number of objects. Methods. The technique is applied to a sample of 137 PNe located between -5 and 5 degrees in Galactic latitude, and between 29.52 and 215.49 degrees in longitude. The characteristics of the distance-extinction method and the main sources of errors are carefully discussed. Results. The data on the extinction of the PNe available in the literature, complemented by new observations, allow us to determine extinction distances for 70 PNe. A comparison with statistical distance scales from different authors is presented.

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IPHAS extinction distances to planetary nebulae

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