List of white dwarfs: Difference between revisions
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| [[Sirius B|Sirius B]] |
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| Sirius B is also the |
| Sirius B is also the second white dwarf discovered. It is part of the [[Sirius]] system. |
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| <ref name=AotU-12.5ly/><ref name=BBC-2005-12-14/><ref name=NWU-WCAS-DavidTaylor-WD>{{cite web |title= White Dwarf Stars Near The Earth |url= http://faculty.wcas.northwestern.edu/~infocom/The%20Website/plates/WD.pdf |author= David Taylor |date= 2012 |work= The Life and Death of Stars |publisher= Weinberg College of Arts and Sciences - Northwestern University }}</ref><ref name=SolStation-WD10pc>{{cite web |url= http://www.solstation.com/stars/pc10wd.htm |title= White dwarfs within 10 parsecs |date= 2011 |publisher= Sol Station }}</ref> |
| <ref name=AotU-12.5ly/><ref name=BBC-2005-12-14/><ref name=NWU-WCAS-DavidTaylor-WD>{{cite web |title= White Dwarf Stars Near The Earth |url= http://faculty.wcas.northwestern.edu/~infocom/The%20Website/plates/WD.pdf |author= David Taylor |date= 2012 |work= The Life and Death of Stars |publisher= Weinberg College of Arts and Sciences - Northwestern University }}</ref><ref name=SolStation-WD10pc>{{cite web |url= http://www.solstation.com/stars/pc10wd.htm |title= White dwarfs within 10 parsecs |date= 2011 |publisher= Sol Station }}</ref> |
Revision as of 00:20, 29 December 2022
This is a list of exceptional white dwarf stars.
Firsts
These were the first white dwarfs discovered fitting these conditions
Title | Star | Date | Data | Comments | Notes | Refs |
---|---|---|---|---|---|---|
First discovered | Sirius B | 1852 | Sirius system | Sirius B is also the nearest white dwarf (as of 2005) | [1][2] | |
First found in a binary star system | ||||||
First double white dwarf system | LDS 275 | 1944 | L 462-56 system | [3] | ||
First solitary white dwarf | Van Maanen 2 | 1917 | Van Maanen's star is also the nearest solitary white dwarf | [4] | ||
First white dwarf in a planetary system | ||||||
First white dwarf with a planet | WD B1620−26 | 2003 | PSR B1620-26 b (planet) | This planet is a circumbinary planet, which circles both stars in the PSR B1620-26 system | [5][6] | |
First singular white dwarf with a planet | WD 1145+017 | 2015 | WD 1145+017 b | Planet is extremely small and is disintegrating. | ||
First white dwarf that is a pulsar | AR Scorpii A | 2016 | The star is in a binary system with a red dwarf | [7] |
Extremes
These are the white dwarfs which are currently known to fit these conditions
Title | Star | Date | Data | Comments | Notes | Refs |
---|---|---|---|---|---|---|
Nearest | Sirius | 1852 | 8.6 ly (2.6 pc) | Sirius B is also the first white dwarf discovered. | [1][2] | |
Farthest | SN UDS10Wil progenitor | 2013 | 10,000,000,000Ly z=1.914 | SN Wilson is a type-Ia supernova whose progenitor was a white dwarf | [8][9][10] | |
Oldest | WD 0343+247 SDSS J110217.48+411315.4 |
2012 | 12 Gy (tied) | |||
Youngest | SDSS J0003+0718 | 2011 | < 13 My | provisional estimate | ||
Highest surface temperature | RX J0439.8−6809 | 2015 | 250,000 K (250,000 °C; 450,000 °F) | This star is located in the Milky Way's galactic halo, in the field of the Large Magellanic Cloud | [11][12] | |
Lowest surface temperature | LSPM J1403+4533 | 2010 | 2,670 K (2,400 °C; 4,350 °F) | Quite a large margin of error (1,500 K (1,230 °C; 2,240 °F)) | [13] | |
Most luminous | ||||||
Least luminous | PSR J2222-0137 B | 2014 | too dim to observe | |||
Brightest apparent | Sirius | 1852 | 8.44 (V) | |||
Dimmest apparent | PSR J2222-0137 B | 2014 | too dim to observe | |||
Most massive (contender) | RE J0317-853 | 1998 | 1.35 M☉ | |||
Most massive (contender) | ZTF J1901+1458 | 2020 | 1.35 M☉ | |||
Least massive | SDSS J091709.55+463821.8 | 2007 | 0.17 M☉ | |||
Largest | Z Andromedae B | 0.265±0.095 R☉ | ||||
Smallest | ZTF J1901+1458 | 2021 | 0.003 R☉ |
Nearest
Star | Distance | Comments | Notes | Refs | |
---|---|---|---|---|---|
Sirius B | 8.58 ly (2.63 pc) | Sirius B is also the second white dwarf discovered. It is part of the Sirius system. | [1][2][14][15] | ||
Procyon B | 11.43 ly (3.50 pc) | Part of Procyon system | [14][15] | ||
van Maanen's Star | 14.04 ly (4.30 pc) | [14][15] | |||
GJ 440 | 15.09 ly (4.63 pc) | [14] | |||
40 Eridani B | 16.25 ly (4.98 pc) | Part of 40 Eridani system | [14][15] | ||
Stein 2051 B | 18.06 ly (5.54 pc) | Part of Stein 2051 system | [14][15] | ||
LP 44-113 | 20.0 ly (6.1 pc) | [15] | |||
G 99-44 | 20.9 ly (6.4 pc) | [15] | |||
L 97-12 | 25.8 ly (7.9 pc) | [15] | |||
Wolf 489 | 26.7 ly (8.2 pc) | [15] |
Notes
- SDSS J1228+1040, A white dwarf with disk of debris.
References
- ^ a b c Atlas of the Universe, "The Universe within 12.5 Light Years: The Nearest Stars", Richard Powell, 30 July 2006 (accessed 2010-11-01)
- ^ a b c BBC News, "Hubble finds mass of white dwarf", Christine McGourty, 14 December 2005 (accessed 2010-11-01)
- ^ W. J. Luyten (September 1944). "Note on the Double White Dwarf L 462-56 = LDS 275". Astrophysical Journal. 100: 202. Bibcode:1944ApJ...100..202L. doi:10.1086/144658.
- ^ Schatzman, Évry (1958), White Dwarfs, North Holland Publishing Company, p. 2.
- ^ Steinn Sigurdsson; Harvey B. Richer; Brad M. Hansen; Ingrid H. Stairs; Stephen E. Thorsett (July 2003). "A Young White Dwarf Companion to Pulsar B1620-26: Evidence for Early Planet Formation". Science. 301 (5630): 193–196. arXiv:astro-ph/0307339. Bibcode:2003Sci...301..193S. doi:10.1126/science.1086326. PMID 12855802.
- ^ "Looking for planets around white dwarfs". Professor Astronomy. 20 August 2010.
- ^ Hambsch, Franz-Josef. "Amateurs Help Discover Pulsing White Dwarf". Sky and Telescope.
- ^ Jason Major (5 April 2013). "Hubble Spots the Most Distant Supernova Ever". Discovery Channel.
- ^ "CANDELS Finds the Most Distant Type Ia Supernova Yet Observed". Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS). 23 April 2013.
- ^ David O. Jones; Steven A. Rodney; Adam G. Riess; Bahram Mobasher; Tomas Dahlen; Curtis McCully; Teddy F. Frederiksen; Stefano Casertano; Jens Hjorth; Charles R. Keeton; Anton Koekemoer; Louis-Gregory Strolger; Tommy G. Wiklind; Peter Challis; Or Graur; Brian Hayden; Brandon Patel; Benjamin J. Weiner; Alexei V. Filippenko; Peter Garnavich; Saurabh W. Jha; Robert P. Kirshner; Henry C. Ferguson; Norman A. Grogin; Dale Kocevski (2 April 2013). "The Discovery of the Most Distant Known Type Ia Supernova at Redshift 1.914". The Astrophysical Journal. 768 (2) (published May 2013): 166. arXiv:1304.0768. Bibcode:2013ApJ...768..166J. doi:10.1088/0004-637X/768/2/166. 166.
- ^ Universitaet Tübingen (24 November 2015). "The hottest white dwarf in the Galaxy". Science Daily.
- ^ K. Werner; T. Rauch (29 September 2015). "Analysis of HST/COS spectra of the bare C–O stellar core H1504+65 and a high-velocity twin in the Galactic halo". Astronomy and Astrophysics. 584 (published December 2015): A19. arXiv:1509.08942. Bibcode:2015A&A...584A..19W. doi:10.1051/0004-6361/201527261. A19.
- ^ Kilic, Mukremin; Leggett, S. K.; Tremblay, P. -E.; von Hippel, Ted; Bergeron, P.; Harris, Hugh C.; Munn, Jeffrey A.; Williams, Kurtis A.; Gates, Evalyn; Farihi, J. (2010-09-01). "A Detailed Model Atmosphere Analysis of Cool White Dwarfs in the Sloan Digital Sky Survey". The Astrophysical Journal Supplement Series. 190: 77–99. doi:10.1088/0067-0049/190/1/77. ISSN 0067-0049.
- ^ a b c d e f David Taylor (2012). "White Dwarf Stars Near The Earth" (PDF). The Life and Death of Stars. Weinberg College of Arts and Sciences - Northwestern University.
- ^ a b c d e f g h i "White dwarfs within 10 parsecs". Sol Station. 2011.
See also
Wikimedia Commons has media related to white dwarfs.