File:A proplyd in the Lagoon Nebula (eso9708b).jpg
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Summary
DescriptionA proplyd in the Lagoon Nebula (eso9708b).jpg |
English: This photo shows a small sky area around the central star of G5.97-1.17, an ultra-compact HII-region (UCHR) in the Lagoon Nebula. This spectacular interstellar nebula, also known as Messier 8 or M8, is seen in the direction of the southern constellation of Sagittarius. Observations described in [/public/news/eso9708/ eso9708] have shown that this star is surrounded by a proplyd (PROto-PLanetarY Disk). |
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Date | 9 April 1997 (upload date) | ||
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Author | NASA/ESA | ||
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Licensing
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Captions
This photo shows a small sky area around the central star of G5.97-1.17, an ultra-compact HII-region (UCHR) in the Lagoon Nebula.
Items portrayed in this file
depicts
image/jpeg
1,122 pixel
1,093 pixel
334,370 byte
4309c654beee5dd0076c4768530d0cb324dc2059
9 April 1997
2b1l8b7kr689x486894pjxg3igoqeo4vu2w1l40cjr3nx47hyi
File history
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current | 18:37, 24 June 2024 | ![]() | 1,093 × 1,122 (327 KB) | OptimusPrimeBot | #Spacemedia - Upload of https://www.eso.org/public/archives/images/large/eso9708b.jpg via Commons:Spacemedia |
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Metadata
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Source | European Southern Observatory |
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Credit/Provider | NASA/ESA |
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Date and time of data generation | 00:00, 9 April 1997 |
JPEG file comment | This photo shows a small sky area around the central star of G5.97-1.17, an ultra-compact HII-region (UCHR) in the Lagoon Nebula. This spectacular interstellar nebula, also known as Messier 8 or M8, is seen in the direction of the southern constellation of Sagittarius.Observations described in eso9708 have shown that this star is surrounded by a proplyd (PROto-PLanetarY Disk).The image is a colour composite based on HST-WFPC2 images obtained through narrow-band optical filtres, isolating the light of doubly ionized oxygen atoms ([OIII]; blue) and atomic hydrogen (H-alpha; green) and in a far-red band (red). Two more faint stars are seen in this image while the bright star Her 36 is outside the border of the image (its location is at the lower left, at the intersection of the vertical, saturated CCD column and the 45° line caused by the light diffracted in the telescope). |
Software used | Adobe Photoshop CS3 Macintosh |
File change date and time | 01:02, 6 July 2017 |
Date and time of digitizing | 17:48, 18 January 2010 |
Date metadata was last modified | 03:02, 6 July 2017 |
Unique ID of original document | uuid:ADE954B606A911DF9F0196888120B175 |
Copyright status | Copyright status not set |
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Contact information |
Karl-Schwarzschild-Strasse 2 Garching bei München, , D-85748 Germany |
IIM version | 4 |