Zur interstellaren Extinktion am galaktischen Nordpol

The mean interstellar extinction is derived from 55 high‐latitude stars ( b ≧ 60°) of luminosity class V to Āv = − 0 m .002 ± 0 m .020 (m.e.) much smaller than follows from a cosec‐law. In the area under consideration the reddening shows no dependence on galactic latitude. It might be possible, that...

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Published in:Astronomische Nachrichten
Main Author: Pfau, W.
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 1963
Subjects:
Nordpol*
Online Access:http://dx.doi.org/10.1002/asna.19632870302
https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2Fasna.19632870302
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.19632870302
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spelling crwiley:10.1002/asna.19632870302 2024-06-02T08:10:52+00:00 Zur interstellaren Extinktion am galaktischen Nordpol Pfau, W. 1963 http://dx.doi.org/10.1002/asna.19632870302 https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2Fasna.19632870302 https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.19632870302 en eng Wiley http://onlinelibrary.wiley.com/termsAndConditions#vor Astronomische Nachrichten volume 287, issue 3, page 97-102 ISSN 0004-6337 1521-3994 journal-article 1963 crwiley https://doi.org/10.1002/asna.19632870302 2024-05-03T10:49:19Z The mean interstellar extinction is derived from 55 high‐latitude stars ( b ≧ 60°) of luminosity class V to Āv = − 0 m .002 ± 0 m .020 (m.e.) much smaller than follows from a cosec‐law. In the area under consideration the reddening shows no dependence on galactic latitude. It might be possible, that the cosec‐law is not fulfilled to the highest latitudes, and therefore, the value of the extinction at the pole which is derived from such a law is too high. Article in Journal/Newspaper Nordpol* Wiley Online Library Astronomische Nachrichten 287 3 97 102
institution Open Polar
collection Wiley Online Library
op_collection_id crwiley
language English
description The mean interstellar extinction is derived from 55 high‐latitude stars ( b ≧ 60°) of luminosity class V to Āv = − 0 m .002 ± 0 m .020 (m.e.) much smaller than follows from a cosec‐law. In the area under consideration the reddening shows no dependence on galactic latitude. It might be possible, that the cosec‐law is not fulfilled to the highest latitudes, and therefore, the value of the extinction at the pole which is derived from such a law is too high.
format Article in Journal/Newspaper
author Pfau, W.
spellingShingle Pfau, W.
Zur interstellaren Extinktion am galaktischen Nordpol
author_facet Pfau, W.
author_sort Pfau, W.
title Zur interstellaren Extinktion am galaktischen Nordpol
title_short Zur interstellaren Extinktion am galaktischen Nordpol
title_full Zur interstellaren Extinktion am galaktischen Nordpol
title_fullStr Zur interstellaren Extinktion am galaktischen Nordpol
title_full_unstemmed Zur interstellaren Extinktion am galaktischen Nordpol
title_sort zur interstellaren extinktion am galaktischen nordpol
publisher Wiley
publishDate 1963
url http://dx.doi.org/10.1002/asna.19632870302
https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1002%2Fasna.19632870302
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.19632870302
genre Nordpol*
genre_facet Nordpol*
op_source Astronomische Nachrichten
volume 287, issue 3, page 97-102
ISSN 0004-6337 1521-3994
op_rights http://onlinelibrary.wiley.com/termsAndConditions#vor
op_doi https://doi.org/10.1002/asna.19632870302
container_title Astronomische Nachrichten
container_volume 287
container_issue 3
container_start_page 97
op_container_end_page 102
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