Undergrad Detecting Protostars: Light Processing Explained

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Protostars are detected through images taken with filters that capture different wavelengths of light, primarily in the infrared range, as they form within nebulas surrounded by gas and dust. Astronomers analyze these images to identify potential protostars by comparing data from various filters. While some believe that automated processing plays a role, others suggest that targets are selected in advance, and manual processing is often involved afterward. Millimeter wave and radio telescopes can also detect signals that penetrate dust, providing additional insights into protostar activity. Overall, the detection process combines both automated and manual techniques to efficiently identify protostars within nebulas.
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How are protostars detected? I doubt that someone is just looking at a poster of a nebula looking for stars.

I'm guessing the image is ran through some kind of light processing program that looks for... something?

Thanks!
 
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Images are taken through filters that let through different wavelengths of light. Protostars form within nebulas, are surrounded by molecular clouds of gas and dust and typically radiate mostly in the infrared range, so by comparing the images taken through the different filters astronomers can identify which stars are most likely protostars.

nmsurobert said:
I'm guessing the image is ran through some kind of light processing program that looks for... something?

Good question. I'm not sure to be honest.
 
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Drakkith said:
Images are taken through filters that let through different wavelengths of light. Protostars form within nebulas, are surrounded by molecular clouds of gas and dust and typically radiate mostly in the infrared range, so by comparing the images taken through the different filters astronomers can identify which stars are most likely protostars.
Good question. I'm not sure to be honest.

i know we can see them but I doubt that's how they're found. I would guess that the data is processed somehow then the image is looked at once a candidate is found.
 
nmsurobert said:
i know we can see them but I doubt that's how they're found. I would guess that the data is processed somehow then the image is looked at once a candidate is found.

I'm not so sure. Targets for telescope observations are often chosen well in advance, so I could easily see the images first being looked at after only a minimal amount of automated processing. In other words, astronomers would choose a target, such as a nebula, write up the proposal to use the appropriate telescope, and then manually do most of the processing themselves once the images come back.
 
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nmsurobert said:
How are protostars detected? ...

Millimeter wave telescopes. Radio telescopes. Some wavelengths will pass through dust that blocks visible and infrared light. Some gasses flow out of nebula which can indicate that something is happening inside.

nmsurobert said:
...I doubt that someone is just looking at a poster of a nebula looking for stars...

Why not look at nebula?
 
stefan r said:
Why not look at nebula?

it seems like "eye balling" for a protostar is inefficient.
 
nmsurobert said:
it seems like "eye balling" for a protostar is inefficient.

I'm not sure to be honest. Narrowing the sky down to just nebulas vastly reduces the number of stars to look at, but I don't know if there is still some sort of automated process in the pipeline.
 

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