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Sh2-207 / Sh2-208, Eddie Bagwell

Sh2-207 / Sh2-208

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Sh2-207 / Sh2-208, Eddie Bagwell

Sh2-207 / Sh2-208

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Description

Two Sharpless targets in this frame from the Constellation Camelopardalis.
Sh2-207 is the larger Nebula on the right and the smaller one to its left is Sh2-208.

1959 - While searching the photo plates of the Palomar Observatory Sky Survey made with the 48-inch Schmidt telescope, the American astronomer Stewart Sharpless came across the two emission nebulae Sh 2-207 and Sh 2-208 and published them in 1959 together with a total of 313 H-II Regions in his catalog.

1961 - The Soviet astronomer Boris Aleksandrovich Vorontsov-Velyaminov suggested that the faint, round nebula (Sh 2-207) could be a typical type IIIb planetary nebula because of the well-defined ring structure.

1967 - Two Czech astronomers Luboš Perek and Luboš Kohoutek listed the nebula in their Catalogue of Galactic Planetary Nebulae under the designation PK 151+2.1.

1976 - Spectroscopic studies showed that Sh 2-207 is more of an H-II region.

2000 - It is reissued as a misclassified PN and probable H-II region.

Present - Sharpless 2-207 is a star-forming region, similar to a miniature version of the Rosette Nebula. The age of the star cluster located in the western part of the nebula has been estimated at about 2-3 million years. The smaller H-II region Sharpless 2-208 is at about the same distance.

Thanks, Eddie

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