最冷恆星列表
最冷恆星列表將恆星以及棕矮星按溫度降低順序排列,其中還包括溫度低於2,000K的恆星。
列表
恆星名稱 | 溫度
(K) |
光譜類型 | 距離(光年) | 註解 |
---|---|---|---|---|
WISE 0855–0714 | 285 | Y4 | ±0.039 7.426 | [1] |
WISE 0336-0143B[2] | ±10 295[3] | Y1? | 32.7[4] | 光譜類型尚未公佈,但如果我們假設MIRIF480M與W2相似,並使用柯克帕特里克等人2012年的圖13,則光譜類型應在Y1[5]可能是晚期的光譜類型。 |
WISEA 0830+2837 | 300-350[6] | >Y1[4] | 26.87[4] | 不確定視差和光譜類型是估計的 |
CWISEP 0238-1332 | ±79 367[4] | >Y1 | 58.66 | 不確定視差和光譜類型是估計的 |
CWISEP 0402-2651 | ±79 367[4] | >Y1 | 39.53 | 不確定視差和光譜類型是估計的 |
WISEU 0503-5648[4] | ±79 367 | >Y1 | 33.18 | 光譜類型是估計的 |
CWISEP 0940+5233[4] | ±79 367 | >Y1 | 43.49 | 不確定視差和光譜類型是估計的 |
WISEA 1257+7153[4] | ±79 367 | >Y1 | 54.18 | 光譜類型是估計的 |
CWISEP J1446−2317[4] | ±79 367 | >Y1 | 37.75 | 不確定視差和光譜類型是估計的 |
WISEA 1930-2059[4] | ±79 367 | >Y1 | 30.67 | 光譜類型是估計的 |
CWISEP 1935-1546[4] | ±79 367 | >Y1 | 47.06 | 光譜類型是估計的 |
CWISEP 2230+2549[4] | ±79 367 | >Y1 | 52.44 | 不確定視差和光譜類型是估計的 |
CWISEP 2256+4002[4] | ±79 367 | >Y1 | 32.04 | 光譜類型是估計的 |
WISE 0825+2805[4] | ±88 376 | Y0.5 | 21.37 | |
WD 0806-661B[4] | ±88 377 | Y1 | 62.80 | 光譜類型是估計的 |
WISE 0350-5658[4] | ±88 388 | Y1 | 18.49 | |
WISEA 2354+0240[4] | ±88 388 | Y1 | 24.97 | |
WISE 2209+2711[4] | ±88 389 | Y0: | 20.17 | |
WISE 0647-6232[4] | ±88 393 | Y1 | 32.78 | |
WISEPA 1541-2250[4] | ±88 395 | Y1 | 19.54 | |
WISE 1828+2650 | ±88 406[4] | Y2V[7] | 32.5 | 溫度可能會更低。如果它是聯雙星,它的成員可能冷到275-350K左右[8]。 |
WISE 0535-7500[4] | ±88 410 | >=Y1: | 47.48 | |
WISE 1405+5534 | ±88 411[4] | Y0.5(pec?)[4] | 20.62 | |
CWISEP 0321+6932[4] | ±79 412 | Y0.5 | 47.61 | 光譜類型是估計的 |
WISE 1639-6847[4] | ±88 412 | Y0pec | 14.85 | |
CWISEP 2356-4814[4] | ±79 412 | Y0.5 | 56.62 | 光譜類型是估計的 |
WISE 0336-0143A[2] | ±24 440[9] | Y0[4] | 32.7[4] | |
WISEPA 1738+2732[4] | ±88 450 | Y0 | 24.92 | |
WISEPA 0410+1502[4] | ±88 451 | Y0 | 21.56 | |
WISE 2220-3628[4] | ±88 452 | Y0 | 34.15 | |
WISE 1534-1043 | ±77 453[10] | sdY? | 53 | 可能是暈棕矮星 |
WISE 1206+8401[4] | ±88 454 | Y0 | 38.51 | |
WISE 0146+4234B[4] | ±79 460 | Y0 | 63.09 | |
WISEA 0302-5817[4] | ±79 460 | Y0: | 54.45 | |
CWISEP 0634+5049[4] | ±79 460 | Y0 | 52.61 | 光譜類型是估計的 |
CWISEP 0859+5349[4] | ±79 460 | Y0 | 60.62 | 光譜類型是估計的 |
CWISE 0925-4720[4] | ±79 460 | Y0 | 34.96 | 光譜類型是估計的 |
CWISEP 0938+0634[4] | ±79 460 | Y0 | 61.31 | 不確定的視差和光譜類型是估計的 |
CWISEP J1047+5457[4] | ±79 460 | Y0 | 43.37 | 光譜類型是估計的 |
CWISE 1121-6232[4] | ±79 460 | Y0 | 33.69 | 光譜類型是估計的 |
WISEA 1141-3326[4] | ±79 460 | Y0 | 31.36 | |
WISE 1217+1626 B | ±79 460[4] | Y0-0.5 | 33 | |
CWISE 1531-3306[4] | ±79 460 | Y0 | 55.37 | 光譜類型是估計的 |
WISENF 1936+0408[4] | ±79 460 | Y0 | 28.64 | 光譜類型是估計的 |
CWISEP 2011-4812[4] | ±79 460 | Y0 | 45.94 | 光譜類型是估計的 |
WISEA 2243-1458[4] | ±79 460 | Y0 | 47,75 | 光譜類型是估計的 |
WISE 1112-3857[4] | ±88 461 | T9 | 31.79 | |
WISE 0734-7157[4] | ±88 462 | Y0 | 43.78 | |
WISE 0713-2917[4] | ±88 464 | Y0 | 29.84 | |
WISEPC 2056+1459[4] | ±88 464 | Y0 | 23.16 | |
WISE 0304-2705[4] | ±88 465 | Y0~pec | 44.62 | |
WISE 0359-5401 | +16 −18 467[11] |
Y0[4] | 44.31[4] | |
WISE 0943+3607[4] | ±88 468 | T9.5 | 33.59 | |
WISE 0833+0052[4] | ±88 472 | (sd)T9 | 40.92 | 可能是次矮星 |
WISE 1542+2230[4] | ±88 472 | T9.5 | 38.69 | |
WISE 0811-8051[4] | ±88 479 | T9.5: | 32.91 | |
WISEPA 2134-7137[4] | ±88 481 | T9~pec | 29.73 | 可能是次矮星 |
WISE 2212-6931[4] | ±88 487 | T9 | 40.47 | |
WISEPA 0751-7634[4] | ±88 492 | T9 | 33.32 | |
WISE 0335+4310[4] | ±88 492 | T9 | 38.46 | |
2MASS 0939-2448 A/B | 650[12] | T8 | ±0.4 17.4 | |
奎宿增三 B | 810 ± 50 | T7.5V | ±0.02 36.32 | [13] |
2M 1237+6526 | 850[14] | T6.5 | 46 | |
2MASS J0348−6022 | 880 | T7[15] | 27.2 | |
GD 165 B | 1,755[16] | L4[17] | 109 | |
仙后座S | 1,800[18] | S3,4–S5,8 | ±300 3,100 | |
小獅座RW | 1,800[19] | C4,3[20] | 1,053[21] | |
英仙座V384 | 1,820[22] | N | ||
DENIS-P J1058.7−1548 | 1,850[23] | L3 | 49 | |
天龍座T | 1,850[22] | C6,2e | ||
V346 Puppis | 1,875[22] | C | ||
2MASS J0523-1403 | 1,939[24] | L2.5V | 41.62 | 2023年已知最冷的主序帶恆星。 |
御夫座S | 1,940[22] | C-N5+ | ||
天鵝座V1426 | 1,975[22] | C7,2e |
相關條目
參考資料
- ^ Luhman, K. L.; Tremblin, P.; Alves de Oliveira, C.; Birkmann, S. M.; Baraffe, I.; Chabrier, G.; Manjavacas, E.; Parker, R. J.; Valenti, J. JWST/NIRSpec Observations of the Coldest Known Brown Dwarf*. The Astronomical Journal. 2023-12-05, 167 (1): 5. ISSN 0004-6256. arXiv:2311.17316 . doi:10.3847/1538-3881/ad0b72 .
- ^ 2.0 2.1 Calissendorff, Per; De Furio, Matthew; Meyer, Michael; Albert, Loïc; Aganze, Christian; Ali-Dib, Mohamad; Bardalez Gagliuffi, Daniella C.; Baron, Frederique; Beichman, Charles A.; Burgasser, Adam J.; Cushing, Michael C.; Faherty, Jacqueline Kelly; Fontanive, Clémence; Gelino, Christopher R.; Gizis, John E. JWST/NIRCam Discovery of the First Y+Y Brown Dwarf Binary: WISE J033605.05-014350.4. The Astrophysical Journal. 2023-04-01, 947 (2): L30. Bibcode:2023ApJ...947L..30C. ISSN 0004-637X. arXiv:2303.16923 . doi:10.3847/2041-8213/acc86d .
- ^ Leggett, S. K.; Tremblin, Pascal. The First Y Dwarf Data From JWST Show That Dynamic and Diabatic Processes Regulate Cold Brown Dwarf Atmospheres. The Astrophysical Journal. 25 Sep 2023, 959 (2): 86. Bibcode:2023ApJ...959...86L. arXiv:2309.14567 . doi:10.3847/1538-4357/acfdad .
- ^ 4.00 4.01 4.02 4.03 4.04 4.05 4.06 4.07 4.08 4.09 4.10 4.11 4.12 4.13 4.14 4.15 4.16 4.17 4.18 4.19 4.20 4.21 4.22 4.23 4.24 4.25 4.26 4.27 4.28 4.29 4.30 4.31 4.32 4.33 4.34 4.35 4.36 4.37 4.38 4.39 4.40 4.41 4.42 4.43 4.44 4.45 4.46 4.47 4.48 4.49 4.50 4.51 4.52 4.53 4.54 4.55 4.56 4.57 4.58 4.59 4.60 4.61 Kirkpatrick, J. Davy; Gelino, Christopher R.; Faherty, Jacqueline K.; Meisner, Aaron M.; Caselden, Dan; Schneider, Adam C.; Marocco, Federico; Cayago, Alfred J.; Smart, R. L.; Eisenhardt, Peter R.; Kuchner, Marc J.; Wright, Edward L.; Cushing, Michael C.; Allers, Katelyn N.; Gagliuffi, Daniella C. Bardalez. The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs. The Astrophysical Journal Supplement Series. 2021-03-01, 253 (1): 7. Bibcode:2021ApJS..253....7K. ISSN 0067-0049. S2CID 227126954. arXiv:2011.11616 . doi:10.3847/1538-4365/abd107 .
- ^ Kirkpatrick, J. Davy; Gelino, Christopher R.; Cushing, Michael C.; Mace, Gregory N.; Griffith, Roger L.; Skrutskie, Michael F.; Marsh, Kenneth A.; Wright, Edward L.; Eisenhardt, Peter R.; McLean, Ian S.; Mainzer, Amanda K.; Burgasser, Adam J.; Tinney, C. G.; Parker, Stephen; Salter, Graeme. Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function. The Astrophysical Journal. 2012-07-01, 753 (2): 156. Bibcode:2012ApJ...753..156K. ISSN 0004-637X. arXiv:1205.2122 . doi:10.1088/0004-637X/753/2/156 .
- ^ Bardalez Gagliuffi, Daniella C.; Faherty, Jacqueline K.; Schneider, Adam C.; Meisner, Aaron; Caselden, Dan; Colin, Guillaume; Goodman, Sam; Kirkpatrick, J. Davy; Kuchner, Marc; Gagné, Jonathan; Logsdon, Sarah E.; Burgasser, Adam J.; Allers, Katelyn; Debes, John; Wisniewski, John. WISEA J083011.95+283716.0: A Missing Link Planetary-mass Object. The Astrophysical Journal. 2020-06-01, 895 (2): 145. Bibcode:2020ApJ...895..145B. ISSN 0004-637X. arXiv:2004.12829 . doi:10.3847/1538-4357/ab8d25 .
- ^ Beichman, Charles A.; Gelino, Christopher R.; Kirkpatrick, J. Davy; Barman, Travis S.; Marsh, Kenneth A.; Cushing, Michael C.; Wright, E. L. The Coldest Brown Dwarf (Or Free Floating Planet)?: The Y Dwarf WISE 1828+2650. The Astrophysical Journal. 2013-01-29, 764 (1): 101. Bibcode:2013ApJ...764..101B. ISSN 0004-637X. S2CID 118575478. arXiv:1301.1669 . doi:10.1088/0004-637X/764/1/101.
- ^ Cushing, Michael C.; Schneider, Adam C.; Kirkpatrick, J. Davy; Morley, Caroline V.; Marley, Mark S.; Gelino, Christopher R.; Mace, Gregory N.; Wright, Edward L.; Eisenhardt, Peter R.; Skrutskie, Michael F.; Marsh, Kenneth A. An Improved Near-infrared Spectrum of the Archetype Y Dwarf WISEP J182831.08+265037.8. The Astrophysical Journal. 2021-10-01, 920 (1): 20. Bibcode:2021ApJ...920...20C. ISSN 0004-637X. arXiv:2107.00506 . doi:10.3847/1538-4357/ac12cb .
- ^ Leggett, S. K.; Tremblin, Pascal. The First Y Dwarf Data From JWST Show That Dynamic and Diabatic Processes Regulate Cold Brown Dwarf Atmospheres. The Astrophysical Journal. 25 Sep 2023, 959 (2): 86. Bibcode:2023ApJ...959...86L. arXiv:2309.14567 . doi:10.3847/1538-4357/acfdad .
- ^ Meisner, Aaron M.; Leggett, S. K.; Logsdon, Sarah E.; Schneider, Adam C.; Tremblin, Pascal; Phillips, Mark. Exploring the Extremes: Characterizing a New Population of Old and Cold Brown Dwarfs. The Astronomical Journal. 2023-08-01, 166 (2): 57. Bibcode:2023AJ....166...57M. ISSN 0004-6256. arXiv:2301.09817 . doi:10.3847/1538-3881/acdb68 .
- ^ Beiler, Samuel A.; Cushing, Michael C.; Kirkpatrick, J. Davy; Schneider, Adam C.; Mukherjee, Sagnick; Marley, Mark S. The First JWST Spectral Energy Distribution of a Y Dwarf. The Astrophysical Journal. 2023-07-01, 951 (2): L48. Bibcode:2023ApJ...951L..48B. ISSN 0004-637X. arXiv:2306.11807 . doi:10.3847/2041-8213/ace32c .
- ^ Leggett, Sandy K.; Cushing, Michael C.; Saumon, Didier; Marley, Mark S.; Roellig, Thomas L.; Warren, Stephen J.; Burningham, Ben; Jones, Hugh R. A.; Kirkpatrick, J. Davy; Lodieu, Nicolas; Lucas, Philip W.; Mainzer, Amy K.; Martín, Eduardo L.; McCaughrean, Mark J.; Pinfield, David J.; Sloan, Gregory C.; Smart, Richard L.; Tamura, Motohide; Van Cleve, Jeffrey E. The Physical Properties of Four ~600 K T Dwarfs. The Astrophysical Journal. 2009, 695 (2): 1517–1526. Bibcode:2009ApJ...695.1517L. S2CID 44050900. arXiv:0901.4093 . doi:10.1088/0004-637X/695/2/1517.
- ^ Luhman, K. L.; Patten, B. M.; Marengo, M.; Schuster, M. T.; Hora, J. L.; Ellis, R. G.; Stauffer, J. R.; Sonnett, S. M.; Winston, E.; Gutermuth, R. A.; Megeath, S. T.; Backman, D. E.; Henry, T. J.; Werner, M. W.; Fazio, G. G. Discovery of Two T Dwarf Companions with the Spitzer Space Telescope. The Astrophysical Journal. January 2007, 654 (1): 570–579. Bibcode:2007ApJ...654..570L. ISSN 0004-637X. arXiv:astro-ph/0609464 . doi:10.1086/509073 .
- ^ Liebert & Burgasser. On the Nature of the Unique Hα-emitting T Dwarf 2MASS J12373919+6526148. Astronomy & Astrophysics. 2007, 655 (1): 522–527. Bibcode:2007ApJ...655..522L. S2CID 18852560. arXiv:astro-ph/0609793 . doi:10.1086/509882.
- ^ Tannock, Megan E.; Metchev, Stanimir; Heinze, Aren; Miles-Páez, Paulo A.; Gagné, Jonathan; Burgasser, Adam; Marley, Mark S.; Apai, Dániel; Suárez, Genaro; Plavchan, Peter. Weather on Other Worlds. V. The Three Most Rapidly Rotating Ultra-Cool Dwarfs. The Astronomical Journal. 2021-05-01, 161 (5): 224. Bibcode:2021AJ....161..224T. ISSN 0004-6256. S2CID 232105126. arXiv:2103.01990 . doi:10.3847/1538-3881/abeb67 .
- ^ Filippazzo, Joseph C.; Rice, Emily L.; Faherty, Jacqueline; Cruz, Kelle L.; Van Gordon, Mollie M.; Looper, Dagny L. Fundamental Parameters and Spectral Energy Distributions of Young and Field Age Objects with Masses Spanning the Stellar to Planetary Regime. The Astrophysical Journal. 2015-09-10, 810 (2): 158. Bibcode:2015ApJ...810..158F. ISSN 1538-4357. S2CID 89611607. arXiv:1508.01767 . doi:10.1088/0004-637X/810/2/158.
- ^ Kirkpatrick, J. Davy; Reid, I. Neill; Liebert, James; Cutri, Roc M.; Nelson, Brant; Beichman, Charles A.; Dahn, Conard C.; Monet, David G.; Gizis, John E.; Skrutskie, Michael F. Dwarfs Cooler than M: The Definition of Spectral Type L Using Discoveries from the 2 Micron All-Sky Survey (2MASS). The Astrophysical Journal. 1999-07-01, 519 (2): 802–833. Bibcode:1999ApJ...519..802K. ISSN 0004-637X. S2CID 73569208. doi:10.1086/307414 .
- ^ Ramstedt, S.; Olofsson, H. The 12CO/13CO ratio in AGB stars of different chemical type - Connection to the 12C/13C ratio and the evolution along the AGB. Astronomy & Astrophysics. 2014-06-01, 566: A145. ISSN 0004-6361. arXiv:1405.6404 . doi:10.1051/0004-6361/201423721 (英语).
- ^ Ramstedt, S.; Olofsson, H. The 12CO/13CO ratio in AGB stars of different chemical type - Connection to the 12C/13C ratio and the evolution along the AGB. Astronomy & Astrophysics. 2014-06-01, 566: A145. ISSN 0004-6361. arXiv:1405.6404 . doi:10.1051/0004-6361/201423721 (英语).
- ^ Cohen, M. Circumstellar envelopes and the evolution of carbon stars.. Monthly Notices of the Royal Astronomical Society. 1979-03-01, 186 (4): 837–852. Bibcode:1979MNRAS.186..837C. ISSN 0035-8711. doi:10.1093/mnras/186.4.837 .
- ^ Bailer-Jones, C. A. L.; Rybizki, J.; Fouesneau, M.; Demleitner, M.; Andrae, R. Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3. The Astronomical Journal. 2021-03-01, 161 (3): 147. Bibcode:2021AJ....161..147B. ISSN 0004-6256. arXiv:2012.05220 . doi:10.3847/1538-3881/abd806 . Data about this star can be seen here.
- ^ 22.0 22.1 22.2 22.3 22.4 Bergeat, J.; Chevallier, L. The mass loss of C-rich giants. Astronomy and Astrophysics. 2005, 429: 235–246. Bibcode:2005A&A...429..235B. S2CID 56424665. arXiv:astro-ph/0601366 . doi:10.1051/0004-6361:20041280.
- ^ Heinze, Aren N.; Metchev, Stanimir; Apai, Daniel; Flateau, Davin; Kurtev, Radostin; Marley, Mark; Radigan, Jacqueline; Burgasser, Adam J.; Artigau, Étienne; Plavchan, Peter. Weather on Other Worlds I: Detection of Periodic Variability in the L3 Dwarf DENIS-P J1058.7-1548 with Precise Multi-Wavelength Photometry. The Astrophysical Journal. 2013-04-08, 767 (2): 173. Bibcode:2013ApJ...767..173H. ISSN 0004-637X. S2CID 29406867. arXiv:1303.2948 . doi:10.1088/0004-637X/767/2/173.
- ^ Filippazzo, Joseph C.; Rice, Emily L.; Faherty, Jacqueline; Cruz, Kelle L.; Van Gordon, Mollie M.; Looper, Dagny L. Fundamental Parameters and Spectral Energy Distributions of Young and Field Age Objects with Masses Spanning the Stellar to Planetary Regime. The Astrophysical Journal. 2015-09-10, 810 (2): 158. Bibcode:2015ApJ...810..158F. ISSN 1538-4357. arXiv:1508.01767 . doi:10.1088/0004-637X/810/2/158.