Gezegenimsi bulutsu (Turkish Wikipedia)
Analysis of information sources in references of the Wikipedia article "Gezegenimsi bulutsu" in Turkish language version.
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archive.org
- Osterbrock, Donald E.; Ferland, G. J. (2005), Ferland, G. J. (Ed.), Astrophysics of gaseous nebulae and active galactic nuclei, University Science Books, ISBN 978-1-891389-34-4
- Observations astronomiques, faites à Toulouse (Astronomical observations, made in Toulouse). Avignon: J. Aubert; (and Paris: Laporte, etc.). 1777.
arxiv.org
- Miszalski et al. 2011 Miszalski, B.; Jones, D.; Rodríguez-Gil, P.; Boffin, H. M. J.; Corradi, R. L. M.; Santander-García, M. (2011), "Discovery of close binary central stars in the planetary nebulae NGC 6326 and NGC 6778", Astronomy and Astrophysics, cilt 531, ss. A158, arXiv:1105.5731 $2, Bibcode:2011A&A...531A.158M, doi:10.1051/0004-6361/201117084
- Frankowski & Soker 2009 Frankowski, Adam; Soker, Noam (November 2009), "Very late thermal pulses influenced by accretion in planetary nebulae", New Astronomy, 14 (8), ss. 654-8, arXiv:0903.3364 $2, Bibcode:2009NewA...14..654F, doi:10.1016/j.newast.2009.03.006,
A planetary nebula (PN) is an expanding ionized circumstellar cloud that was ejected during the asymptotic giant branch (AGB) phase of the stellar progenitor.
- Zijlstra, A. (2015). "Planetary nebulae in 2014: A review of research" (PDF). Revista Mexicana de Astronomía y Astrofísica. 51: 221-230. arXiv:1506.05508 $2. 9 Ekim 2022 tarihinde kaynağından (PDF) arşivlendi.
- Hora et al. 2004 Hora, Joseph L.; Latter, William B.; Allen, Lori E.; Marengo, Massimo; Deutsch, Lynne K.; Pipher, Judith L. (September 2004), "Infrared Array Camera (IRAC) Observations of Planetary Nebulae" (PDF), Astrophysical Journal Supplement Series, 154 (1), ss. 296-301, arXiv:astro-ph/0405614 $2, Bibcode:2004ApJS..154..296H, doi:10.1086/422820, 28 Temmuz 2023 tarihinde kaynağından arşivlendi (PDF), erişim tarihi: 28 Temmuz 2023
- Reed et al. 1999 Reed, Darren S.; Balick, Bruce; Hajian, Arsen R.; Klayton, Tracy L.; Giovanardi, Stefano; Casertano, Stefano; Panagia, Nino; Terzian, Yervant (November 1999), "Hubble Space Telescope Measurements of the Expansion of NGC 6543: Parallax Distance and Nebular Evolution", Astronomical Journal, 118 (5), ss. 2430-41, arXiv:astro-ph/9907313 $2, Bibcode:1999AJ....118.2430R, doi:10.1086/301091
- Maciel, Costa & Idiart 2009 Maciel, W. J.; Costa, R. D. D.; Idiart, T. E. P. (October 2009), "Planetary nebulae and the chemical evolution of the Magellanic Clouds", Revista Mexicana de Astronomía y Astrofísica, cilt 45, ss. 127-37, arXiv:0904.2549 $2, Bibcode:2009RMxAA..45..127M,
These objects are produced by low and intermediate mass stars, with main sequence masses roughly between 0.8 and 8 M⊙, and present a reasonably large age and metallicity spread.
books.google.com
- Kwok 2000 Kwok, Sun (2000), The origin and evolution of planetary nebulae, Cambridge University Press, ISBN 0-521-62313-8, 2 Mart 2012 tarihinde kaynağından arşivlendi (Chapter 1 can be downloaded here.)
- Krause 1961 Krause, Arthur (1961), Astronomy, Oliver and Boyd, s. 187
- Harpaz 1994 Harpaz, Amos (1994), Stellar Evolution, A K Peters, Ltd., ISBN 978-1-56881-012-6
caltech.edu
authors.library.caltech.edu
- Hora et al. 2004 Hora, Joseph L.; Latter, William B.; Allen, Lori E.; Marengo, Massimo; Deutsch, Lynne K.; Pipher, Judith L. (September 2004), "Infrared Array Camera (IRAC) Observations of Planetary Nebulae" (PDF), Astrophysical Journal Supplement Series, 154 (1), ss. 296-301, arXiv:astro-ph/0405614 $2, Bibcode:2004ApJS..154..296H, doi:10.1086/422820, 28 Temmuz 2023 tarihinde kaynağından arşivlendi (PDF), erişim tarihi: 28 Temmuz 2023
doi.org
- Miszalski et al. 2011 Miszalski, B.; Jones, D.; Rodríguez-Gil, P.; Boffin, H. M. J.; Corradi, R. L. M.; Santander-García, M. (2011), "Discovery of close binary central stars in the planetary nebulae NGC 6326 and NGC 6778", Astronomy and Astrophysics, cilt 531, ss. A158, arXiv:1105.5731 $2, Bibcode:2011A&A...531A.158M, doi:10.1051/0004-6361/201117084
- Frankowski & Soker 2009 Frankowski, Adam; Soker, Noam (November 2009), "Very late thermal pulses influenced by accretion in planetary nebulae", New Astronomy, 14 (8), ss. 654-8, arXiv:0903.3364 $2, Bibcode:2009NewA...14..654F, doi:10.1016/j.newast.2009.03.006,
A planetary nebula (PN) is an expanding ionized circumstellar cloud that was ejected during the asymptotic giant branch (AGB) phase of the stellar progenitor.
- Huggins & Miller 1864 Huggins, W.; Miller, W. A. (1864), "On the Spectra of some of the Nebulae", Philosophical Transactions of the Royal Society of London, cilt 154, ss. 437-44, Bibcode:1864RSPT..154..437H, doi:10.1098/rstl.1864.0013
- Kwok 2005 Kwok, Sun (June 2005), "Planetary Nebulae: New Challenges in the 21st Century", Journal of the Korean Astronomical Society, 38 (2), ss. 271-8, Bibcode:2005JKAS...38..271K, doi:10.5303/JKAS.2005.38.2.271
- Hora et al. 2004 Hora, Joseph L.; Latter, William B.; Allen, Lori E.; Marengo, Massimo; Deutsch, Lynne K.; Pipher, Judith L. (September 2004), "Infrared Array Camera (IRAC) Observations of Planetary Nebulae" (PDF), Astrophysical Journal Supplement Series, 154 (1), ss. 296-301, arXiv:astro-ph/0405614 $2, Bibcode:2004ApJS..154..296H, doi:10.1086/422820, 28 Temmuz 2023 tarihinde kaynağından arşivlendi (PDF), erişim tarihi: 28 Temmuz 2023
- Kwok et al. 2006 Kwok, Sun; Koning, Nico; Huang, Hsiu-Hui; Churchwell, Edward (2006), Barlow, M. J.; Méndez, R. H. (Ed.), "Planetary nebulae in the GLIMPSE survey", Proceedings of the International Astronomical Union, Symposium #234, Planetary Nebulae in our Galaxy and Beyond, Cambridge: Cambridge University Press, 2 (S234), ss. 445-6, Bibcode:2006IAUS..234..445K, doi:10.1017/S1743921306003668 ,
Planetary nebulae (PNs) have high dust content and radiate strongly in the infrared. For young PNs, the dust component accounts for about one third of the total energy output of the nebulae (Zhang & Kwok 1991). The typical color temperatures of PNs are between 100 and 200 K, and at λ >5 μm, dust begins to dominate over bound-free emission from the ionized component. Although PNs are traditionally discovered through examination of photographic plates or Hα surveys, PNs can also be identified in infrared surveys by searching for red objects with a rising spectrum between 4–10 μm.
- Reed et al. 1999 Reed, Darren S.; Balick, Bruce; Hajian, Arsen R.; Klayton, Tracy L.; Giovanardi, Stefano; Casertano, Stefano; Panagia, Nino; Terzian, Yervant (November 1999), "Hubble Space Telescope Measurements of the Expansion of NGC 6543: Parallax Distance and Nebular Evolution", Astronomical Journal, 118 (5), ss. 2430-41, arXiv:astro-ph/9907313 $2, Bibcode:1999AJ....118.2430R, doi:10.1086/301091
- Wood (2004). "Long Secondary Periods in Pulsating Asymptotic Giant Branch Stars: An Investigation of Their Origin". The Astrophysical Journal. 604 (2): 800. doi:10.1086/382123.
ghostarchive.org
- Zijlstra, A. (2015). "Planetary nebulae in 2014: A review of research" (PDF). Revista Mexicana de Astronomía y Astrofísica. 51: 221-230. arXiv:1506.05508 $2. 9 Ekim 2022 tarihinde kaynağından (PDF) arşivlendi.
harvard.edu
adsabs.harvard.edu
- Miszalski et al. 2011 Miszalski, B.; Jones, D.; Rodríguez-Gil, P.; Boffin, H. M. J.; Corradi, R. L. M.; Santander-García, M. (2011), "Discovery of close binary central stars in the planetary nebulae NGC 6326 and NGC 6778", Astronomy and Astrophysics, cilt 531, ss. A158, arXiv:1105.5731 $2, Bibcode:2011A&A...531A.158M, doi:10.1051/0004-6361/201117084
- Frankowski & Soker 2009 Frankowski, Adam; Soker, Noam (November 2009), "Very late thermal pulses influenced by accretion in planetary nebulae", New Astronomy, 14 (8), ss. 654-8, arXiv:0903.3364 $2, Bibcode:2009NewA...14..654F, doi:10.1016/j.newast.2009.03.006,
A planetary nebula (PN) is an expanding ionized circumstellar cloud that was ejected during the asymptotic giant branch (AGB) phase of the stellar progenitor.
- Moore 2007 Moore, S. L. (October 2007), "Observing the Cat's Eye Nebula", Journal of the British Astronomical Association, 117 (5), ss. 279-80, Bibcode:2007JBAA..117R.279M
- Huggins & Miller 1864 Huggins, W.; Miller, W. A. (1864), "On the Spectra of some of the Nebulae", Philosophical Transactions of the Royal Society of London, cilt 154, ss. 437-44, Bibcode:1864RSPT..154..437H, doi:10.1098/rstl.1864.0013
- Kwok 2005 Kwok, Sun (June 2005), "Planetary Nebulae: New Challenges in the 21st Century", Journal of the Korean Astronomical Society, 38 (2), ss. 271-8, Bibcode:2005JKAS...38..271K, doi:10.5303/JKAS.2005.38.2.271
- Hora et al. 2004 Hora, Joseph L.; Latter, William B.; Allen, Lori E.; Marengo, Massimo; Deutsch, Lynne K.; Pipher, Judith L. (September 2004), "Infrared Array Camera (IRAC) Observations of Planetary Nebulae" (PDF), Astrophysical Journal Supplement Series, 154 (1), ss. 296-301, arXiv:astro-ph/0405614 $2, Bibcode:2004ApJS..154..296H, doi:10.1086/422820, 28 Temmuz 2023 tarihinde kaynağından arşivlendi (PDF), erişim tarihi: 28 Temmuz 2023
- Kwok et al. 2006 Kwok, Sun; Koning, Nico; Huang, Hsiu-Hui; Churchwell, Edward (2006), Barlow, M. J.; Méndez, R. H. (Ed.), "Planetary nebulae in the GLIMPSE survey", Proceedings of the International Astronomical Union, Symposium #234, Planetary Nebulae in our Galaxy and Beyond, Cambridge: Cambridge University Press, 2 (S234), ss. 445-6, Bibcode:2006IAUS..234..445K, doi:10.1017/S1743921306003668 ,
Planetary nebulae (PNs) have high dust content and radiate strongly in the infrared. For young PNs, the dust component accounts for about one third of the total energy output of the nebulae (Zhang & Kwok 1991). The typical color temperatures of PNs are between 100 and 200 K, and at λ >5 μm, dust begins to dominate over bound-free emission from the ionized component. Although PNs are traditionally discovered through examination of photographic plates or Hα surveys, PNs can also be identified in infrared surveys by searching for red objects with a rising spectrum between 4–10 μm.
- Reed et al. 1999 Reed, Darren S.; Balick, Bruce; Hajian, Arsen R.; Klayton, Tracy L.; Giovanardi, Stefano; Casertano, Stefano; Panagia, Nino; Terzian, Yervant (November 1999), "Hubble Space Telescope Measurements of the Expansion of NGC 6543: Parallax Distance and Nebular Evolution", Astronomical Journal, 118 (5), ss. 2430-41, arXiv:astro-ph/9907313 $2, Bibcode:1999AJ....118.2430R, doi:10.1086/301091
- Maciel, Costa & Idiart 2009 Maciel, W. J.; Costa, R. D. D.; Idiart, T. E. P. (October 2009), "Planetary nebulae and the chemical evolution of the Magellanic Clouds", Revista Mexicana de Astronomía y Astrofísica, cilt 45, ss. 127-37, arXiv:0904.2549 $2, Bibcode:2009RMxAA..45..127M,
These objects are produced by low and intermediate mass stars, with main sequence masses roughly between 0.8 and 8 M⊙, and present a reasonably large age and metallicity spread.
hubblesite.org
- Hubblesite.org 1997 Hubble Witnesses the Final Blaze of Glory of Sun-Like Stars, Hubblesite.org - Space Telescope Science Institute (STScI) for NASA, 17 Aralık 1997, 12 Haziran 2018 tarihinde kaynağından arşivlendi, erişim tarihi: 10 Haziran 2018
klima-luft.de
- Wolfgang Steinicke. "Antoine Darquier de Pellepoix". 25 Ocak 2003 tarihinde kaynağından arşivlendi. Erişim tarihi: 9 Haziran 2018.
nasa.gov
- "Messier 27 (The Dumbbell Nebula)". nasa.gov. 19 Ekim 2017. 10 Nisan 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 28 Temmuz 2023.
seds.org
messier.seds.org
- SEDS 2013 Planetary Nebulae, SEDS, 9 Eylül 2013, 10 Kasım 2013 tarihinde kaynağından arşivlendi, erişim tarihi: 10 Kasım 2013
smithsonianmag.com
- Daley, Jason (8 Mayıs 2018). "The Sun Will Produce a Beautiful Planetary Nebula When It Dies". Smithsonian Magazine (İngilizce). 8 Mayıs 2018 tarihinde kaynağından arşivlendi. Erişim tarihi: 30 Mart 2020.
unam.mx
astroscu.unam.mx
- Zijlstra, A. (2015). "Planetary nebulae in 2014: A review of research" (PDF). Revista Mexicana de Astronomía y Astrofísica. 51: 221-230. arXiv:1506.05508 $2. 9 Ekim 2022 tarihinde kaynağından (PDF) arşivlendi.
web.archive.org
- "Messier 27 (The Dumbbell Nebula)". nasa.gov. 19 Ekim 2017. 10 Nisan 2020 tarihinde kaynağından arşivlendi. Erişim tarihi: 28 Temmuz 2023.
- Wolfgang Steinicke. "Antoine Darquier de Pellepoix". 25 Ocak 2003 tarihinde kaynağından arşivlendi. Erişim tarihi: 9 Haziran 2018.
- Daley, Jason (8 Mayıs 2018). "The Sun Will Produce a Beautiful Planetary Nebula When It Dies". Smithsonian Magazine (İngilizce). 8 Mayıs 2018 tarihinde kaynağından arşivlendi. Erişim tarihi: 30 Mart 2020.
- Kwok 2000 Kwok, Sun (2000), The origin and evolution of planetary nebulae, Cambridge University Press, ISBN 0-521-62313-8, 2 Mart 2012 tarihinde kaynağından arşivlendi (Chapter 1 can be downloaded here.)
- SEDS 2013 Planetary Nebulae, SEDS, 9 Eylül 2013, 10 Kasım 2013 tarihinde kaynağından arşivlendi, erişim tarihi: 10 Kasım 2013
- Hubblesite.org 1997 Hubble Witnesses the Final Blaze of Glory of Sun-Like Stars, Hubblesite.org - Space Telescope Science Institute (STScI) for NASA, 17 Aralık 1997, 12 Haziran 2018 tarihinde kaynağından arşivlendi, erişim tarihi: 10 Haziran 2018
- Hora et al. 2004 Hora, Joseph L.; Latter, William B.; Allen, Lori E.; Marengo, Massimo; Deutsch, Lynne K.; Pipher, Judith L. (September 2004), "Infrared Array Camera (IRAC) Observations of Planetary Nebulae" (PDF), Astrophysical Journal Supplement Series, 154 (1), ss. 296-301, arXiv:astro-ph/0405614 $2, Bibcode:2004ApJS..154..296H, doi:10.1086/422820, 28 Temmuz 2023 tarihinde kaynağından arşivlendi (PDF), erişim tarihi: 28 Temmuz 2023