File Download
There are no files associated with this item.
Links for fulltext
(May Require Subscription)
- Publisher Website: 10.1017/S1743921306003218
- Scopus: eid_2-s2.0-33845526976
- Find via
Supplementary
-
Citations:
- Scopus: 0
- Appears in Collections:
Article: 400 new planetary nebulae in the galactic bulge
Title | 400 new planetary nebulae in the galactic bulge |
---|---|
Authors | |
Keywords | Planetary nebulae Galactic bulge |
Issue Date | 2006 |
Citation | Proceedings of the International Astronomical Union, 2006, v. 2, n. 234, p. 355-356 How to Cite? |
Abstract | About 500 MASH(Macquarie/AAO/Strasbourg Hα planetary nebula, project) PNe were discovered towards the galactic bulge (Parker et al. 2006). For 405 MASH PNe with a diameter < 35 arcsec, we obtain surface brightness, diameter and dynamical age of the nebulae. From line intensity ratios of 133 GBPN observed with the 6dF device, we obtain their density and ionized mass, and their central star temperatures. We discover 15 bipolar and/or nitrogen-rich GBPNe having probably massive stellar progenitors (Peyaud, 2005). © 2006 International Astronomical Union. |
Persistent Identifier | http://hdl.handle.net/10722/208868 |
ISSN | 2023 SCImago Journal Rankings: 0.121 |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Acker, Agnès | - |
dc.contributor.author | Peyaud, Alan E J | - |
dc.contributor.author | Parker, Quentin A. | - |
dc.date.accessioned | 2015-03-23T02:02:00Z | - |
dc.date.available | 2015-03-23T02:02:00Z | - |
dc.date.issued | 2006 | - |
dc.identifier.citation | Proceedings of the International Astronomical Union, 2006, v. 2, n. 234, p. 355-356 | - |
dc.identifier.issn | 1743-9213 | - |
dc.identifier.uri | http://hdl.handle.net/10722/208868 | - |
dc.description.abstract | About 500 MASH(Macquarie/AAO/Strasbourg Hα planetary nebula, project) PNe were discovered towards the galactic bulge (Parker et al. 2006). For 405 MASH PNe with a diameter < 35 arcsec, we obtain surface brightness, diameter and dynamical age of the nebulae. From line intensity ratios of 133 GBPN observed with the 6dF device, we obtain their density and ionized mass, and their central star temperatures. We discover 15 bipolar and/or nitrogen-rich GBPNe having probably massive stellar progenitors (Peyaud, 2005). © 2006 International Astronomical Union. | - |
dc.language | eng | - |
dc.relation.ispartof | Proceedings of the International Astronomical Union | - |
dc.subject | Planetary nebulae | - |
dc.subject | Galactic bulge | - |
dc.title | 400 new planetary nebulae in the galactic bulge | - |
dc.type | Article | - |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1017/S1743921306003218 | - |
dc.identifier.scopus | eid_2-s2.0-33845526976 | - |
dc.identifier.volume | 2 | - |
dc.identifier.issue | 234 | - |
dc.identifier.spage | 355 | - |
dc.identifier.epage | 356 | - |
dc.identifier.eissn | 1743-9221 | - |
dc.identifier.issnl | 1743-9213 | - |