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HD 106461


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BP Octantis - a Variable Am Star
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A photometric study of some AM stars
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A survey for southern Delta Scuti variable stars
Twenty-nine field stars have been tested photoelectrically forshort-period variability. Eighteen of these stars have spectral typesbetween A2 and F5 and are not Am stars; of these, six have beendiscovered to be variable and one is a suspected variable. HD 185969,with a period of 0.361 day, has the longest known period for a star ofthe Delta Scuti type. The predominance of discovered variables withamplitudes close to the detection limit is suggestive of most stars inthe instability strip being pulsators.

Is HR 5491 Really a Pulsating AM Star?
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1972PASP...84..443B&db_key=AST

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Observation and Astrometry data

Constellation:Oktant
Right ascension:12h18m46.06s
Declination:-88°24'53.7"
Apparent magnitude:6.617
Distance:193.798 parsecs
Proper motion RA:-32.2
Proper motion Dec:10.8
B-T magnitude:6.544
V-T magnitude:6.611

Catalogs and designations:
Proper Names
HD 1989HD 106461
TYCHO-2 2000TYC 9520-59-1
USNO-A2.0USNO-A2 0000-00945465
HIPHIP 60041

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