Skip to main content Accessibility help
×
Home

Emission Line Properties of Seyfert 1 Type AGN from RASS

  • D. W. Xu (a1) (a2), S. Komossa (a1), J. Y. Wei (a2), X. Z. Zheng (a2) and Y. Qian (a3)...

Abstract

We present the optical emission line properties of a sample of 155 bright X-ray selected ROSAT Seyfert 1 type AGN. The measured properties are gathered for correlation analysis. The strong correlations between Hβ redshift, flux ratios of Fe II to Hβ broad component and [O III] to Hβ narrow component are found.

    • Send article to Kindle

      To send this article to your Kindle, first ensure no-reply@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about sending to your Kindle. Find out more about sending to your Kindle.

      Note you can select to send to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be sent to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

      Find out more about the Kindle Personal Document Service.

      Emission Line Properties of Seyfert 1 Type AGN from RASS
      Available formats
      ×

      Send article to Dropbox

      To send this article to your Dropbox account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Dropbox.

      Emission Line Properties of Seyfert 1 Type AGN from RASS
      Available formats
      ×

      Send article to Google Drive

      To send this article to your Google Drive account, please select one or more formats and confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your <service> account. Find out more about sending content to Google Drive.

      Emission Line Properties of Seyfert 1 Type AGN from RASS
      Available formats
      ×

Copyright

References

Hide All
Boroson, T.A. 2002, ApJ, 565, 78
Boroson, T.A., & Green, R.F. 1992, ApJS, 80, 109
Voges, W., Aschenbach, B., Boller, Th., et al. 1996, IAU Circ. 6420
Wei, J.Y., Xu, D.W., Dong, X.Y., & Hu, J.Y. 1999, A&AS, 139, 575

Emission Line Properties of Seyfert 1 Type AGN from RASS

  • D. W. Xu (a1) (a2), S. Komossa (a1), J. Y. Wei (a2), X. Z. Zheng (a2) and Y. Qian (a3)...

Metrics

Full text views

Total number of HTML views: 0
Total number of PDF views: 0 *
Loading metrics...

Abstract views

Total abstract views: 0 *
Loading metrics...

* Views captured on Cambridge Core between <date>. This data will be updated every 24 hours.

Usage data cannot currently be displayed