by Ann » Mon May 31, 2021 6:25 pm
bystander wrote: ↑Mon May 31, 2021 4:36 pm
The Eponymous NGC 691
ESA Hubble Picture of the Week | 2021 May 31
This image features the spiral galaxy
NGC 691, imaged in fantastic detail by Hubble’s Wide Field Camera 3 (
WFC3). This galaxy is the eponymous member of the
NGC 691 galaxy group, a group of gravitationally bound galaxies that lie about 120 million light-years from Earth.
Objects such as NGC 691 are observed by Hubble using a range of filters. Each filter only allows certain wavelengths of light to reach Hubble’s WFC3. The images collected using different filters are then coloured by specialised visual artists who can make informed choices about which colour best corresponds to which filter. By combining the coloured images from individual filters, a full-colour image of the astronomical object can be recreated. In this way, we can get remarkably good insight into the nature and appearance of these objects.
I'm not entirely impressed with the colors of the version of the picture of GC 691 that we can see in bystander's post.
In my opinion, the (inner) arms of NGC 691 in bystander's post are too tightly wound, too regular and too lacking in obvious major sites of star formation to be as blue as they appear to be in the image in bystander's post. The color of the arms doesn't fit their morphology!
The picture I'm posting shows a much more "reasonable" image of NGC 691, in my opinion. Note that the inner arms are barely blue. There is an underlying population of old yellow stars in them, "overlaid" with a relatively rich population of bluish but modest stars like Sirius and Vega. The overall color is neutral.
Further out, NGC 691 runs out of (large populations of) old yellow stars. The lack of "incredible multitudes" of stars makes the outer regions quite dark, but they are lit up by a number of widely scattered blue knots of high-mass star formation.
Ann
[quote=bystander post_id=313798 time=1622478961 user_id=112005]
[url=https://esahubble.org/images/potw2122a/][size=125][b][i]The Eponymous NGC 691[/i][/b][/size][/url]
ESA Hubble Picture of the Week | 2021 May 31
[quote]
[float=left][img3="Credit: ESA/Hubble & NASA, A. Riess
Acknowledgement: M. Zamani"]https://cdn.spacetelescope.org/archives/images/screen/potw2122a.jpg[/img3][/float]This image features the spiral galaxy [url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC+691]NGC 691[/url], imaged in fantastic detail by Hubble’s Wide Field Camera 3 ([url=https://esahubble.org/about/general/instruments/wfc3/]WFC3[/url]). This galaxy is the eponymous member of the [url=https://en.wikipedia.org/wiki/NGC_691]NGC 691[/url] galaxy group, a group of gravitationally bound galaxies that lie about 120 million light-years from Earth.
Objects such as NGC 691 are observed by Hubble using a range of filters. Each filter only allows certain wavelengths of light to reach Hubble’s WFC3. The images collected using different filters are then coloured by specialised visual artists who can make informed choices about which colour best corresponds to which filter. By combining the coloured images from individual filters, a full-colour image of the astronomical object can be recreated. In this way, we can get remarkably good insight into the nature and appearance of these objects. [/quote]
[/quote]
[float=right][img3="NGC 691. Image credit: ESA/Hubble & NASA, A. Riess et al."]https://www.nasa.gov/sites/default/files/styles/full_width_feature/public/thumbnails/image/potw2008a.jpg[/img3][/float]
I'm not entirely impressed with the colors of the version of the picture of GC 691 that we can see in bystander's post.
In my opinion, the (inner) arms of NGC 691 in bystander's post are too tightly wound, too regular and too lacking in obvious major sites of star formation to be as blue as they appear to be in the image in bystander's post. The color of the arms doesn't fit their morphology!
The picture I'm posting shows a much more "reasonable" image of NGC 691, in my opinion. Note that the inner arms are barely blue. There is an underlying population of old yellow stars in them, "overlaid" with a relatively rich population of bluish but modest stars like Sirius and Vega. The overall color is neutral.
Further out, NGC 691 runs out of (large populations of) old yellow stars. The lack of "incredible multitudes" of stars makes the outer regions quite dark, but they are lit up by a number of widely scattered blue knots of high-mass star formation.
Ann