| Hercules X-1 | has eclipse duration 0.24 days (in X-rays) |  |
| is a part of Hercules |  |
| has eccentricity e < 0.1 |  |
| has distance 5 kpc |  |
| has synonym 3U 1653+35 |  |
| has orbital period 1.7 days |  |
| has definition An X-ray pulsar, a member of an occulting binary system. The visible component has been identified as the blue variable HZ Herculis, whose spectrum varies from late A or early F to B. Her X- l has a pulsation period of 1.2378 seconds, presumably its rotation period, and exhibits a 35-day quasi-periodicity in the X-ray region (but not in the optical). It is probably a rotating neutron star in a circular orbit with a mass of about 0.7 Msun, which is accreting matter from HZ Her. The orbital period is stable, but the pulsation period is speeding up at a rate of about 1 part in 105 per year. The X-ray eclipse lasts 0.24 days. |  |
| is an instance of X-ray pulsar |  |
| is an instance of eclipsing binary |  |
| periodic variable | has period |  |
| pulsar | has acronym PSR |  |
| binary star | has number of stars 2 |  |
| variable | has name designated with - R, S, T, U, V, W, X, Y, or Z and the genitive of the latin constellation name
- RR, RS, RT, RU, RV, RW, RX, RY, or RZ and the genitive of the latin constellation name when the single letter designations are exhausted
- AA...AZ, BB...BZ, etc. (omitting J), which ends with QQ...QZ and the genitive of the latin constellation namewhen the RR...RZ designations are exhausted
- V 335, V 336, etc., when the double letter designations are exhausted
|  |
| has observational problem some difficulty in distinguishing between various kinds |  |
| has observable variation time scale within a period of decades |  |
| has light curve |  |
| has optical brightness variation 0.2 magnitudes or greater |  |
| has amplitude |  |
| star system | has abundance half the stars in the solar neighborhood are members of star systems |  |
| star | has star surface temperature |  |
| has spectral type |  |
| has V magnitude |  |
| has B magnitude |  |
| has U magnitude |  |
| has position on celestial sphere from the point of view of Earth |  |
| has parallax from the point of view of Earth's orbit |  |
| has proper motion |  |
| has radiation at surface which is diffused out from the hotter core |  |
| has energy source gravitational contraction and or fusion |  |
| has energy production which takes place primarily within the core |  |
| has surface density which depends on luminosity class |  |
| has surface temperature greater than 1000 Kelvin |  |
| has apparent magnitude |  |
| has absolute magnitude |  |
| has age |  |
| has catalog star catalog |  |
| has material hydrogen, helium |  |
| has velocity determined from proper motion and radial velocity |  |
| has mass greater than 0.08 the sun's mass |  |
| massive compact halo object | is a part of halo |  |
| celestial body | has spectra |  |
| dark matter | is a part of dark halo |  |
| hypothetical particle | has acceptance status hypothetical |  |
| physical object | has location or center of gravity |  |
| has angular momentum |  |
| has momentum |  |
| has temperature |  |
| has volume |  |
| has extent |  |
| particle | obeys uncertainty principle |  |
| has frequency inversely proportional to the wavelength |  |
| has wavelength inversely proportional to its momentum |  |
| has charge |  |