Messier 108 (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Messier 108" in English language version.

refsWebsite

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9harvard.edu

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6arxiv.org

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5doi.org

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4semanticscholar.org

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3wis-tns.org

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1caltech.edu

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1oup.com

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1seds.org

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1messier-objects.com

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1nasa.gov

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1handle.net

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arxiv.org

Sorce, J. G.; et al. (2014). "From Spitzer Galaxy photometry to Tully–Fisher distances". Monthly Notices of the Royal Astronomical Society. 444 (1): 527–541. arXiv:1408.0729. doi:10.1093/mnras/stu1450.
Wang, Q. Daniel; et al. (2003). "Chandra Observation of the Edge-on Galaxy NGC 3556 (M 108): Violent Galactic Disk-halo Interaction Revealed". The Astrophysical Journal. 598 (2): 969–981. arXiv:astro-ph/0308150. Bibcode:2003ApJ...598..969W. doi:10.1086/379010. S2CID 49349099.
Rhode, Katherine L.; et al. (2007). "Global Properties of the Globular Cluster Systems of Four Spiral Galaxies". Astronomical Journal. 134 (4): 1403–1418. arXiv:0708.1166. Bibcode:2007AJ....134.1403R. doi:10.1086/521397. S2CID 15834447.
Gopal-Krishna; Irwin, Judith A. (2000). "Radio jet-blown neutral hydrogen supershells in spiral galaxies?". Astronomy and Astrophysics. 361: 888–894. arXiv:astro-ph/0008251. Bibcode:2000A&A...361..888G.
Satyapal, S.; et al. (2008). "Spitzer Uncovers Active Galactic Nuclei Missed by Optical Surveys in Seven Late-Type Galaxies". Astrophysical Journal. 677 (2): 926–942. arXiv:0801.2759. Bibcode:2008ApJ...677..926S. doi:10.1086/529014. S2CID 16050838.
Jencson, Jacob E.; et al. (2018). "SPIRITS 16tn in NGC 3556: A Heavily Obscured and Low-luminosity Supernova at 8.8 Mpc". The Astrophysical Journal. 863 (1): 20. arXiv:1803.00574. Bibcode:2018ApJ...863...20J. doi:10.3847/1538-4357/aacf8b. hdl:10150/631110. S2CID 56398022.

caltech.edu

ned.ipac.caltech.edu

"NASA/IPAC Extragalactic Database". Results for NGC 3556. Retrieved 30 March 2022.

doi.org

Sorce, J. G.; et al. (2014). "From Spitzer Galaxy photometry to Tully–Fisher distances". Monthly Notices of the Royal Astronomical Society. 444 (1): 527–541. arXiv:1408.0729. doi:10.1093/mnras/stu1450.
Wang, Q. Daniel; et al. (2003). "Chandra Observation of the Edge-on Galaxy NGC 3556 (M 108): Violent Galactic Disk-halo Interaction Revealed". The Astrophysical Journal. 598 (2): 969–981. arXiv:astro-ph/0308150. Bibcode:2003ApJ...598..969W. doi:10.1086/379010. S2CID 49349099.
Rhode, Katherine L.; et al. (2007). "Global Properties of the Globular Cluster Systems of Four Spiral Galaxies". Astronomical Journal. 134 (4): 1403–1418. arXiv:0708.1166. Bibcode:2007AJ....134.1403R. doi:10.1086/521397. S2CID 15834447.
Satyapal, S.; et al. (2008). "Spitzer Uncovers Active Galactic Nuclei Missed by Optical Surveys in Seven Late-Type Galaxies". Astrophysical Journal. 677 (2): 926–942. arXiv:0801.2759. Bibcode:2008ApJ...677..926S. doi:10.1086/529014. S2CID 16050838.
Jencson, Jacob E.; et al. (2018). "SPIRITS 16tn in NGC 3556: A Heavily Obscured and Low-luminosity Supernova at 8.8 Mpc". The Astrophysical Journal. 863 (1): 20. arXiv:1803.00574. Bibcode:2018ApJ...863...20J. doi:10.3847/1538-4357/aacf8b. hdl:10150/631110. S2CID 56398022.

handle.net

hdl.handle.net

Jencson, Jacob E.; et al. (2018). "SPIRITS 16tn in NGC 3556: A Heavily Obscured and Low-luminosity Supernova at 8.8 Mpc". The Astrophysical Journal. 863 (1): 20. arXiv:1803.00574. Bibcode:2018ApJ...863...20J. doi:10.3847/1538-4357/aacf8b. hdl:10150/631110. S2CID 56398022.

harvard.edu

ui.adsabs.harvard.edu

Using an assumed distance of 7.1 Megaparsec to Messier 108, based on a 1986 study.[1]
This is the angular size of the feature as it appears on the sky. The physical size depends on the distance to Messier 108, which is more difficult to measure. At the time of the study that discovered this feature (in 2003),^[9] the accepted distance to Messier 108 was based on a 1988 work,[2] which gave a value of 14.1 Megaparsec (Mpc). This has been substantially revised down to 8.8 Mpc in a 2014 study.^[3] At 14.1 Mpc, an angular size of 2.6 arcminutes would correspond to a physical size of $2.6/60\cdot \pi /180\cdot 14100=10.7$ kpc, or roughly 10 kiloparsec (kpc), which is the value given in the 2003 study. Using the more recent distance estimate, this would be $2.6/60\cdot \pi /180\cdot 8800=6.7$ kpc. Compare the list of distance measurements in the NASA/IPAC Extragalactic Database.^[2]
Tully, R. B.; Fisher, J. R. (1977). "A new method of determining distances to galaxies". Astronomy and Astrophysics. 54 (3): 661–673. Bibcode:1977A&A....54..661T.
Wang, Q. Daniel; et al. (2003). "Chandra Observation of the Edge-on Galaxy NGC 3556 (M 108): Violent Galactic Disk-halo Interaction Revealed". The Astrophysical Journal. 598 (2): 969–981. arXiv:astro-ph/0308150. Bibcode:2003ApJ...598..969W. doi:10.1086/379010. S2CID 49349099.
Rhode, Katherine L.; et al. (2007). "Global Properties of the Globular Cluster Systems of Four Spiral Galaxies". Astronomical Journal. 134 (4): 1403–1418. arXiv:0708.1166. Bibcode:2007AJ....134.1403R. doi:10.1086/521397. S2CID 15834447.
Gopal-Krishna; Irwin, Judith A. (2000). "Radio jet-blown neutral hydrogen supershells in spiral galaxies?". Astronomy and Astrophysics. 361: 888–894. arXiv:astro-ph/0008251. Bibcode:2000A&A...361..888G.
Satyapal, S.; et al. (2008). "Spitzer Uncovers Active Galactic Nuclei Missed by Optical Surveys in Seven Late-Type Galaxies". Astrophysical Journal. 677 (2): 926–942. arXiv:0801.2759. Bibcode:2008ApJ...677..926S. doi:10.1086/529014. S2CID 16050838.
Jencson, Jacob E.; et al. (2018). "SPIRITS 16tn in NGC 3556: A Heavily Obscured and Low-luminosity Supernova at 8.8 Mpc". The Astrophysical Journal. 863 (1): 20. arXiv:1803.00574. Bibcode:2018ApJ...863...20J. doi:10.3847/1538-4357/aacf8b. hdl:10150/631110. S2CID 56398022.

cbat.eps.harvard.edu

Marsden, Brian G. (12 February 1969). "Circular No. 2131". Central Bureau for Astronomical Telegrams. Smithsonian Astrophysical Observatory. Retrieved 2 December 2024.

messier-objects.com

"Messier 108: Surfboard Galaxy". Messier Objects: Guide to the Bright Galaxies, Nebulae and Clusters Listed in the Messier Catalogue. 26 September 2015.

nasa.gov

science.nasa.gov

"Messier 108". NASA. Retrieved 17 November 2024.

oup.com

academic.oup.com

Sorce, J. G.; et al. (2014). "From Spitzer Galaxy photometry to Tully–Fisher distances". Monthly Notices of the Royal Astronomical Society. 444 (1): 527–541. arXiv:1408.0729. doi:10.1093/mnras/stu1450.

seds.org

messier.seds.org

"Messier 108". SEDS Messier Catalog. Retrieved 30 April 2022.

semanticscholar.org

api.semanticscholar.org

Wang, Q. Daniel; et al. (2003). "Chandra Observation of the Edge-on Galaxy NGC 3556 (M 108): Violent Galactic Disk-halo Interaction Revealed". The Astrophysical Journal. 598 (2): 969–981. arXiv:astro-ph/0308150. Bibcode:2003ApJ...598..969W. doi:10.1086/379010. S2CID 49349099.
Rhode, Katherine L.; et al. (2007). "Global Properties of the Globular Cluster Systems of Four Spiral Galaxies". Astronomical Journal. 134 (4): 1403–1418. arXiv:0708.1166. Bibcode:2007AJ....134.1403R. doi:10.1086/521397. S2CID 15834447.
Satyapal, S.; et al. (2008). "Spitzer Uncovers Active Galactic Nuclei Missed by Optical Surveys in Seven Late-Type Galaxies". Astrophysical Journal. 677 (2): 926–942. arXiv:0801.2759. Bibcode:2008ApJ...677..926S. doi:10.1086/529014. S2CID 16050838.
Jencson, Jacob E.; et al. (2018). "SPIRITS 16tn in NGC 3556: A Heavily Obscured and Low-luminosity Supernova at 8.8 Mpc". The Astrophysical Journal. 863 (1): 20. arXiv:1803.00574. Bibcode:2018ApJ...863...20J. doi:10.3847/1538-4357/aacf8b. hdl:10150/631110. S2CID 56398022.

wis-tns.org

"SN 1969B". Transient Name Server. IAU. Retrieved 2 December 2024.
"SN 2023dbc". Transient Name Server. IAU. Retrieved 2 December 2024.
"AstroNote 2023-66 : SN 2023dbc as a Highly Extinguished Stripped-Envelope Supernova". Transient Name Server. 2023-03-22. Retrieved 2023-04-03.