NSVS 2607629
Simbad link | NSVS 2607629 |
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Source publication | Kjurkchieva, Diana P. (2018) - Observations and Light Curve Solutions of Ultrashort-Period Eclipsing Binaries |
ADS link | 2018PASA...35....8K |
Name in Source publication | NSVS 2607629 |
Orbital period in days (P [d]) | 0.22937 |
Mass ratio (q) | 0.62 |
Mass ratio determination | Photometric |
Type | A |
Has total eclipse? | |
Has spots? | |
Has third light? | |
Has period variation? |
Solver | PHOEBE |
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Orbital period in days (P [d]) | 0.22937 |
Mass ratio (q) | 0.62 |
Orbital inclination in degrees (i [o]) | 80.2 |
Fillout (f) | 0.28 |
Primary temperature in Kelvins (T1 [K]) | 5390 |
Secondary temperature in Kelvins (T2 [K]) | 5168 |
Primary polar radius in units of orbital separation (r1p) | 0.4126 |
Secondary polar radius in units of orbital separation (r2p) | 0.3334 |
Surface potential (Ω) | 2.996 |
Orbital separation in solar radii (a [R]) | 1.66 |
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Primary radius in solar units (R1 [R]) | 0.74 |
Secondary radius in solar units (R2 [R]) | 0.6 |
Primary mass in solar units (M1 [M]) | 0.72 |
Secondary mass in solar units (M2 [M]) | 0.45 |
Primary temperature in kelvins (T1 [K]) | 5390 |
Secondary temperature in Kelvins (T2 [K]) | 5168 |
Primary luminosity in solar units (L1 [L]) | 0.41 |
Secondary luminosity in solar units (L2 [L]) | 0.23 |
Distance in parsecs (d [pc]) | |
Age in gigayears (τ [gyr]) |
Designation | Gaia DR2 841507376028169856 |
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RA | 175:36:21.006 |
DEC | 54:52:49.219248 |
l | 142.5977657 |
b | 59.53412793 |
G magnitude | 12.268148 |
G_bp magnitude | 12.79816 |
G_rp magnitude | 11.594439 |
Radial velocity [km/s] | |
Parallax | 5.602850416 |
Distance [pc] | 178.480581 |
Temperature [K] | 4876 |
Radius [R] | 0.8095788 |
Luminosity [L] | 0.3337857 |
Simbad link | NSVS 2607629 |
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J magnitude | 10.547 |
H magnitude | 10.055 |
K magnitude | 9.959 |
Johnson_U magnitude | |
Johnson_B magnitude | |
Johnson_V magnitude | |
Johnson_R magnitude | |
Johnson_I magnitude | |
Sloan_u magnitude | |
Sloan_g magnitude | 12.2681 |
Sloan_r magnitude | |
Sloan_i magnitude | |
Sloan_z magnitude |