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21-cm observations of the CEP IV star-formation region
The Cep IV star-formation region has been mapped at 21 cm. The resultingH I distribution indicates that the available gas forms a broken ringcoincident with the optical nebulosity. Comparison of this feature withother kinematic data for both stars and gas suggests that sequentialstar formation is an ongoing process in this region.
| A Study of the Cepheus IV Association
Abstract image available at:http://adsabs.harvard.edu/abs/1968ApJS...16..275M
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Observation and Astrometry data
| Constellation: | Kepheus |
| Right ascension: | 23h57m49.75s |
| Declination: | +68°28'28.4" |
| Apparent magnitude: | 10.798 |
| Proper motion RA: | 0.5 |
| Proper motion Dec: | -1.9 |
| B-T magnitude: | 11.554 |
| V-T magnitude: | 10.861 |
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