File:NGC 6302 with (Fe II) Emission.png
Original file (4,767 × 3,147 pixels, file size: 22.61 MB, MIME type: image/png)
Captions
Captions
Summary
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| Description |
New observations from 2019 (Prop 15953/Joel Kastner) reveal [Fe II] emission, shown here in pink, along the edges of the biopolar outflows of this young planetary nebula. I created this image specifically to clearly detail this discovery, deliberately arranging filters and assigning colors that would draw one's eyes to the new emission line data. Hat tip to Bruce Balick for his original idea of removing the stars in the [Fe II] data. Through a strange series of emails I ended up "stealing" this idea, but he seemed happy about it when confession time came. Data from the following proposals were used to create this image: WFC3 ERO: Planetary Nebula Young and Rapidly Evolving: a Panchromatic WFC3 Imaging Study of the Planetary Nebulae NGC 7027 and NGC 6302 Note that stars were manually removed from the F164N/[Fe II] data. Red screen: F164N ([Fe II]) Red: F673N Yellow-Green: F658N Blue: F373N North is 35.20° clockwise from up. |
| Date | |
| Source | NGC 6302 with [Fe II] Emission |
| Author | Judy Schmidt from USA |
Licensing
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This image was originally posted to Flickr by geckzilla at https://flickr.com/photos/54209675@N00/50023499248. It was reviewed on 20 June 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 09:33, 20 June 2020 | | 4,767 × 3,147 (22.61 MB) | Fabian RRRR (talk | contribs) | =={{int:filedesc}}== {{Information |Description=New observations from 2019 (Prop 15953/Joel Kastner) reveal [Fe II] emission, shown here in pink, along the edges of the biopolar outflows of this young planetary nebula. I created this image specifically to clearly detail this discovery, deliberately arranging filters and assigning colors that would draw one's eyes to the new emission line data. Hat tip to Bruce Balick for his original idea of removing the stars in the [Fe II] data. Through a... |
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