WD 2359-434 (Q5176940)

catalog code

2MASS J00021076-4309560

1 reference

23 April 2014

GJ 915

Gliese Catalogue of Nearby Stars

1 reference

retrieved

23 April 2014

WD 2359-434

1 reference

retrieved

23 April 2014

PLX 5808

General Catalogue of Trigonometric Stellar Parallaxes

1 reference

CSI-43-23595

Catalog of Stellar Identifications

1 reference

LFT 1849

Luyten Five-Tenths catalogue

1 reference

LHS 1005

Luyten Half-Second catalogue

1 reference

LPM 901

Luyten Proper-Motion catalogue

1 reference

LTT 9857

Luyten Two-Tenths catalogue

1 reference

UBV 20649

UBV Photoelectric Photometry Catalogue

1 reference

Zkh 356

1 reference

uvby98 986362081

uvbyβ Photoelectric Photometric Catalogue

1 reference

PLX 5808.00

General Catalogue of Trigonometric Stellar Parallaxes

1 reference

NLTT 58832

New Luyten Two-Tenths catalogue

1 reference

BPM 45338

Bruce proper motion survey. The general catalogue. Vol. I, II

1 reference

CF 20541

Catalogue of 20554 faint stars in the Cape astrographic zone -40 to -52 for the equinox of 1900.0, Royal Obs. Cape of Good Hope

1 reference

Ci 20 1474

Catalogue of proper motion stars

1 reference

PM 23596-4325

Catalogs of proper-motion stars. I. Stars brighter than visual magnitude 15 and with annual proper motion of 1" or more

1 reference

imported from Wikimedia project

Gaia DR2 4994877094997259264

1 reference

1 reference

26.7±0.2 light-year

1 reference

Russian Wikipedia

Wikimedia import URL

https://ru.wikipedia.org/?oldid=98810269

8.3351±0.0023 parsec

1 reference

6.1 parsec

1 reference

3D kinematics of white dwarfs from the SPY project. II.

19 parsec

1 reference

A spectroscopic survey and analysis of bright, hydrogen-rich white dwarfs

7.27 parsec

1 reference

The white dwarfs within 20 parsecs of the Sun: kinematics and statistics

parallax

121.02±1.11 milliarcsecond

1 reference

The solar neighborhood. XXI. Parallax results from the CTIOPI 0.9 M program: 20 new members of the 25 parsec white dwarf sample

119.9752±0.0336 milliarcsecond

1 reference

127.4±6.8 milliarcsecond

1 reference

The General Catalogue of Trigonometric Stellar Parallaxes, Fourth Edition

declination component of proper motion

−668.8±7.4 milliarcsecond per year

1 reference

The AllWISE motion survey, part 2

−663.9±0.8 milliarcsecond per year

1 reference

The solar neighborhood. XXI. Parallax results from the CTIOPI 0.9 M program: 20 new members of the 25 parsec white dwarf sample

−686.734±0.036 milliarcsecond per year

1 reference

−731±102 milliarcsecond per year

1 reference

Discoveries from a near-infrared proper motion survey using multi-epoch Two Micron All-Sky Survey data

−724±100 milliarcsecond per year

2 references

Revised coordinates and proper motions of the stars in the Luyten half-second catalog

Low-Luminosity Companions to White Dwarfs

−690±40 milliarcsecond per year

1 reference

The Liverpool-Edinburgh high proper motion survey

right ascension component of proper motion

607.1±8.3 milliarcsecond per year

1 reference

The AllWISE motion survey, part 2

589.4±0.8 milliarcsecond per year

1 reference

The solar neighborhood. XXI. Parallax results from the CTIOPI 0.9 M program: 20 new members of the 25 parsec white dwarf sample

613.639±0.038 milliarcsecond per year

1 reference

682±95 milliarcsecond per year

1 reference

Discoveries from a near-infrared proper motion survey using multi-epoch Two Micron All-Sky Survey data

719±100 milliarcsecond per year

2 references

Revised coordinates and proper motions of the stars in the Luyten half-second catalog

Low-Luminosity Companions to White Dwarfs

650±20 milliarcsecond per year

1 reference

The Liverpool-Edinburgh high proper motion survey

radial velocity

−58.8±10.8 kilometre per second

1 reference

3D kinematics of white dwarfs from the SPY project. II.

spectral class

DAP5.8

1 reference

A spectroscopic survey and analysis of bright, hydrogen-rich white dwarfs

DAP

1 reference

The Solar Neighborhood. XXXIX. Parallax Results from the CTIOPI and NOFS Programs: 50 New Members of the 25 parsec White Dwarf Sample

DA

3 references

High-resolution UVES/VLT spectra of white dwarfs observed for the ESO SN Ia Progenitor Survey

3D kinematics of white dwarfs from the SPY project. II.

High-resolution UVES/VLT spectra of white dwarfs observed for the ESO SNIa progenitor survey (SPY). I

DAs

1 reference

G.P. Kuiper's spectral classifications of proper-motion stars

DAH

1 reference

High-resolution UVES/VLT spectra of white dwarfs observed for the ESO SN Ia Progenitor Survey

13.12

1 reference

23 April 2014

13.05

1 reference

23 April 2014

12.597±0.026

astronomical filter

J band

1 reference

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

12.425±0.023

astronomical filter

H band

1 reference

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

12.445±0.024

astronomical filter

K band

1 reference

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

12.9137±0.0004

1 reference

13.2

3 references

reference URL

http://adsabs.harvard.edu/abs/2008AJ....135.1225H

reference URL

https://arxiv.org/abs/0902.0627

imported from Wikimedia project

Russian Wikipedia

Wikimedia import URL

https://ru.wikipedia.org/?oldid=98810269

metallicity

122

1 reference

1 reference

0.54468497951780 degree

1 reference

declination

−43.16538735508110 degree

1 reference

effective temperature

8,390 kelvin

1 reference

The Solar Neighborhood. XXXIX. Parallax Results from the CTIOPI and NOFS Programs: 50 New Members of the 25 parsec White Dwarf Sample

8,650 kelvin

1 reference

A spectroscopic survey and analysis of bright, hydrogen-rich white dwarfs

8,672 kelvin

1 reference

High-resolution UVES/VLT spectra of white dwarfs observed for the ESO SNIa progenitor survey (SPY). I

8,570 kelvin

1 reference

The white dwarfs within 20 parsecs of the Sun: kinematics and statistics

surface gravity

680,000,000 centimetre per square second

1 reference

High-resolution UVES/VLT spectra of white dwarfs observed for the ESO SNIa progenitor survey (SPY). I

360,000,000 centimetre per square second

1 reference

A spectroscopic survey and analysis of bright, hydrogen-rich white dwarfs

234,000,000 centimetre per square second

1 reference