2mass+j154043.42+ˆ’510135.7 Latitude and Longitude:

Sky map 15h 40m 43.537s, −51° 01′ 35.968″
From Wikipedia, the free encyclopedia
2MASS J15404341−5101357
Observation data
Epoch J2000       Equinox J2000
Constellation Norma
Right ascension 15h 40m 43.537s [1]
Declination −51° 01′ 35.968″ [1]
Apparent magnitude (V) 15.26 [2]
Characteristics
Evolutionary stage main-sequence star [2]
Spectral type M7V [2]
Apparent magnitude (J) 8.96 [3]
Astrometry
Radial velocity (Rv)50.0 [3] km/s
Proper motion (μ) RA: +1.954 [2]  mas/ yr
Dec.: âˆ’0.330 [2]  mas/ yr
Parallax (Ï€)187.7290 Â± 0.0496  mas [4]
Distance17.374 ± 0.005  ly
(5.327 ± 0.001  pc)
Absolute bolometric
magnitude
 (Mbol)
12.81 [2]
Details [2]
Mass0.090±0.010  M
Luminosity0.000603  L
Temperature2621±100  K
Other designations
GJ 12259, [5] 2MASS J154043.42-510135.7, WISEA J154045.67-510139.3, UCAC4 195-119117, Gaia DR2 5985290231327158144
Database references
SIMBAD data
2M1540 is located in the constellation Norma
2M1540 is located in the constellation Norma
2M1540
Location of 2M1540 in the constellation Norma

2MASS J15404341−5101357 (abbreviated 2M1540) is a red dwarf of spectral type M7, located in Norma at approximately 17 light-years from Earth. It is the nearest known M7 dwarf. [2]

Discovery

Its discovery was announced in 2014 by Kirkpatrick et al. [6] and independently by Pérez Garrido et al. [2]

Kirkpatrick and colleagues found a few thousand new high proper motion objects under the AllWISE program of study of images, taken by Wide-field Infrared Survey Explorer (WISE). 2M1540 was one of these high proper motion objects. They named it WISEA J154045.67-510139.3 and assigned it spectral type M6. [6]

Pérez Garrido and colleagues were looking for high proper motion sources in the 2MASS– WISE cross-match. They named it 2MASS J154043.42-510135.7 (2M1540 for short) and classified it as an M7.0±0.5 dwarf. [2]

Since the trigonometric distance of 2M1540 agreed with its spectrophotometric distances, computed for a single object, it was concluded that it is not an equal-mass binary. [2]

References

  1. ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051.
  2. ^ a b c d e f g h i j k Pérez Garrido, A.; Lodieu, N.; Béjar, V. J. S.; Ruiz, M. T.; Gauza, B.; Rebolo, R.; Zapatero Osorio, M. R. (2014). "2MASS J154043.42-510135.7: a new addition to the 5 pc population". Astronomy & Astrophysics. 567: A6. arXiv: 1405.5439. Bibcode: 2014A&A...567A...6P. doi: 10.1051/0004-6361/201423615. S2CID  118704532.
  3. ^ a b Henry, Todd J.; Jao, Wei-Chun; Winters, Jennifer G.; Dieterich, Sergio B.; Finch, Charlie T.; Ianna, Philip A.; Riedel, Adric R.; Silverstein, Michele L.; Subasavage, John P.; Vrijmoet, Eliot Halley (2018), "The Solar Neighborhood XLIV: RECONS Discoveries within 10 parsecs", The Astronomical Journal, 155 (6): 265, arXiv: 1804.07377, Bibcode: 2018AJ....155..265H, doi: 10.3847/1538-3881/aac262, S2CID  53983430
  4. ^ Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv: 2012.01533. Bibcode: 2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657. S2CID  227254300. (Erratum:  doi: 10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  5. ^ Golovin, Alex; Reffert, Sabine; Just, Andreas; Jordan, Stefan; Vani, Akash; Jahreiß, Hartmut (November 2022). "The Fifth Catalogue of Nearby Stars (CNS5)". Astronomy & Astrophysics. 670: A19. arXiv: 2211.01449. Bibcode: 2023A&A...670A..19G. doi: 10.1051/0004-6361/202244250. S2CID  253264922. Catalogue can be accessed here.
  6. ^ a b Kirkpatrick, J. Davy; Schneider, Adam; Fajardo-Acosta, Sergio; Gelino, Christopher R.; Mace, Gregory N.; Wright, Edward L.; Logsdon, Sarah E.; McLean, Ian S.; Cushing, Michael C.; Skrutskie, Michael F.; Eisenhardt, Peter R.; Stern, Daniel; Baloković, Mislav; Burgasser, Adam J.; Faherty, Jacqueline K.; Lansbury, George B.; Rich, J. A.; Skrzypek, Nathalie; Fowler, John W.; Cutri, Roc M.; Masci, Frank J.; Conrow, Tim; Grillmair, Carl J.; McCallon, Howard L.; Beichman, Charles A.; Marsh, Kenneth A. (2014). "The AllWISE Motion Survey and the Quest for Cold Subdwarfs". The Astrophysical Journal. 783 (2): 122. arXiv: 1402.0661. Bibcode: 2014ApJ...783..122K. doi: 10.1088/0004-637X/783/2/122. S2CID  30949660.

2mass+j154043.42+ˆ’510135.7 Latitude and Longitude:

Sky map 15h 40m 43.537s, −51° 01′ 35.968″
From Wikipedia, the free encyclopedia
2MASS J15404341−5101357
Observation data
Epoch J2000       Equinox J2000
Constellation Norma
Right ascension 15h 40m 43.537s [1]
Declination −51° 01′ 35.968″ [1]
Apparent magnitude (V) 15.26 [2]
Characteristics
Evolutionary stage main-sequence star [2]
Spectral type M7V [2]
Apparent magnitude (J) 8.96 [3]
Astrometry
Radial velocity (Rv)50.0 [3] km/s
Proper motion (μ) RA: +1.954 [2]  mas/ yr
Dec.: âˆ’0.330 [2]  mas/ yr
Parallax (Ï€)187.7290 Â± 0.0496  mas [4]
Distance17.374 ± 0.005  ly
(5.327 ± 0.001  pc)
Absolute bolometric
magnitude
 (Mbol)
12.81 [2]
Details [2]
Mass0.090±0.010  M
Luminosity0.000603  L
Temperature2621±100  K
Other designations
GJ 12259, [5] 2MASS J154043.42-510135.7, WISEA J154045.67-510139.3, UCAC4 195-119117, Gaia DR2 5985290231327158144
Database references
SIMBAD data
2M1540 is located in the constellation Norma
2M1540 is located in the constellation Norma
2M1540
Location of 2M1540 in the constellation Norma

2MASS J15404341−5101357 (abbreviated 2M1540) is a red dwarf of spectral type M7, located in Norma at approximately 17 light-years from Earth. It is the nearest known M7 dwarf. [2]

Discovery

Its discovery was announced in 2014 by Kirkpatrick et al. [6] and independently by Pérez Garrido et al. [2]

Kirkpatrick and colleagues found a few thousand new high proper motion objects under the AllWISE program of study of images, taken by Wide-field Infrared Survey Explorer (WISE). 2M1540 was one of these high proper motion objects. They named it WISEA J154045.67-510139.3 and assigned it spectral type M6. [6]

Pérez Garrido and colleagues were looking for high proper motion sources in the 2MASS– WISE cross-match. They named it 2MASS J154043.42-510135.7 (2M1540 for short) and classified it as an M7.0±0.5 dwarf. [2]

Since the trigonometric distance of 2M1540 agreed with its spectrophotometric distances, computed for a single object, it was concluded that it is not an equal-mass binary. [2]

References

  1. ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051.
  2. ^ a b c d e f g h i j k Pérez Garrido, A.; Lodieu, N.; Béjar, V. J. S.; Ruiz, M. T.; Gauza, B.; Rebolo, R.; Zapatero Osorio, M. R. (2014). "2MASS J154043.42-510135.7: a new addition to the 5 pc population". Astronomy & Astrophysics. 567: A6. arXiv: 1405.5439. Bibcode: 2014A&A...567A...6P. doi: 10.1051/0004-6361/201423615. S2CID  118704532.
  3. ^ a b Henry, Todd J.; Jao, Wei-Chun; Winters, Jennifer G.; Dieterich, Sergio B.; Finch, Charlie T.; Ianna, Philip A.; Riedel, Adric R.; Silverstein, Michele L.; Subasavage, John P.; Vrijmoet, Eliot Halley (2018), "The Solar Neighborhood XLIV: RECONS Discoveries within 10 parsecs", The Astronomical Journal, 155 (6): 265, arXiv: 1804.07377, Bibcode: 2018AJ....155..265H, doi: 10.3847/1538-3881/aac262, S2CID  53983430
  4. ^ Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv: 2012.01533. Bibcode: 2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657. S2CID  227254300. (Erratum:  doi: 10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  5. ^ Golovin, Alex; Reffert, Sabine; Just, Andreas; Jordan, Stefan; Vani, Akash; Jahreiß, Hartmut (November 2022). "The Fifth Catalogue of Nearby Stars (CNS5)". Astronomy & Astrophysics. 670: A19. arXiv: 2211.01449. Bibcode: 2023A&A...670A..19G. doi: 10.1051/0004-6361/202244250. S2CID  253264922. Catalogue can be accessed here.
  6. ^ a b Kirkpatrick, J. Davy; Schneider, Adam; Fajardo-Acosta, Sergio; Gelino, Christopher R.; Mace, Gregory N.; Wright, Edward L.; Logsdon, Sarah E.; McLean, Ian S.; Cushing, Michael C.; Skrutskie, Michael F.; Eisenhardt, Peter R.; Stern, Daniel; Baloković, Mislav; Burgasser, Adam J.; Faherty, Jacqueline K.; Lansbury, George B.; Rich, J. A.; Skrzypek, Nathalie; Fowler, John W.; Cutri, Roc M.; Masci, Frank J.; Conrow, Tim; Grillmair, Carl J.; McCallon, Howard L.; Beichman, Charles A.; Marsh, Kenneth A. (2014). "The AllWISE Motion Survey and the Quest for Cold Subdwarfs". The Astrophysical Journal. 783 (2): 122. arXiv: 1402.0661. Bibcode: 2014ApJ...783..122K. doi: 10.1088/0004-637X/783/2/122. S2CID  30949660.

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