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| Query : 2000MNRAS.318....9B |
2000MNRAS.318....9B - Mon. Not. R. Astron. Soc., 318, 9-17 (2000/October-2)
A TiO study of the dwarf nova IP Pegasi.
BEEKMAN G., SOMERS M., NAYLOR T. and HELLIER C.
Abstract (from CDS):
By fitting the phase-resolved spectra around the TiO bands to a mean spectrum, we attempt to isolate the light curve of the secondary star. The resulting light curve has marked deviations from the expected ellipsoidal shape. The largest difference is at phase 0.5, and can be explained as an eclipse of the secondary star by the disc, indicating that the disc is optically thick when viewed at high inclination angles.
Abstract Copyright: 2000, Royal Astronomical Society
Journal keyword(s): binaries: close - binaries: eclipsing - binaries: spectroscopic - stars: fundamental parameters - stars: individual: IP Peg - novae, cataclysmic variables
Simbad objects: 1
| Number of rows : 1 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | V* IP Peg | CV* | 23 23 08.5362249504 | +18 24 59.206884012 | M2 | 395 | 0 |
| Query : 2000MNRAS.318....9B |
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| SV* SVS 2549 | SBC9 1442 | WEB 20444 | AAVSO 2318+17 |
| LAMOST J232308.57+182459.8 | TIC 243129676 | ZTF17aabulaf |
Gaia DR3 2824150286583562496
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2MASS J23230854+1824593
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V* IP Peg
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EQ 2320+181 |
Gaia DR2 2824150286583562496
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References (395 between 1850 and 2026) (Total 395)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). |
Link by name to the catalogue in VizieR :
| 2MASS J23230854+1824593 | V* IP Peg | Gaia DR3 2824150286583562496 | Gaia DR2 2824150286583562496 |
Search by coordinates in Vizier (radius: 5 arcsec)
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