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A Fast Chi-Squared Technique for Period Search of Irregularly Sampled Data
A new, computationally and statistically efficient algorithm, the Fast?2 algorithm (F?2), can find a periodicsignal with harmonic content in irregularly sampled data with nonuniformerrors. The algorithm calculates the minimized ?2 as afunction of frequency at the desired number of harmonics, using fastFourier transforms to provide O(Nlog N) performance. The code for areference implementation is provided.
| New Elements for 80 Eclipsing Binaries VII.
This research presents new elements for 80 eclipsing binaries found withthe help of the ASAS-3, Hipparcos and NSVS databases.
| An Einstein Observatory SAO-based catalog of B-type stars
About 4000 X-ray images obtained with the Einstein Observatory are usedto measure the 0.16-4.0 keV emission from 1545 B-type SAO stars fallingin the about 10 percent of the sky surveyed with the IPC. Seventy-fourdetected X-ray sources with B-type stars are identified, and it isestimated that no more than 15 can be misidentified. Upper limits to theX-ray emission of the remaining stars are presented. In addition tosummarizing the X-ray measurements and giving other relevant opticaldata, the present extensive catalog discusses the reduction process andanalyzes selection effects associated with both SAO catalog completenessand IPC target selection procedures. It is concluded that X-rayemission, at the level of Lx not less than 10 exp 30 ergs/s, is quitecommon in B stars of early spectral types (B0-B3), regardless ofluminosity class, but that emission, at the same level, becomes lesscommon, or nonexistent, in later B-type stars.
| Four-colour and H-beta photometry for early type stars in three southern galactic regions
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1980A&AS...41...85L&db_key=AST
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Observation and Astrometry data
| Constellation: | Zentaur |
| Right ascension: | 14h11m47.99s |
| Declination: | -62°01'34.8" |
| Apparent magnitude: | 7.714 |
| Distance: | 694.444 parsecs |
| Proper motion RA: | -3.5 |
| Proper motion Dec: | -3 |
| B-T magnitude: | 7.738 |
| V-T magnitude: | 7.716 |
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