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Questions about the observed frequency range of the electromagnetic radiation of a celestial object.

2 votes
2 answers
581 views

How to tell whether an optical spectrum is featureless or just with a low S/N?

A featureless spectrum and a spectrum low S/N are very similar. Is there a way to tell the difference between them?
questionhang's user avatar
  • 3,157
14 votes
3 answers
2k views

How to detect emission lines in optical spectra?

Is there any handy module to detect emission lines in a spectrum like one we get from the Sloan Digital Sky Survey (SDSS)? You can see there are many emission lines like Ha,OI in the spectrum below. …
questionhang's user avatar
  • 3,157
2 votes
2 answers
890 views

How do I understand a brown dwarf with a M-type spectrum?

The reason we do not need to create a new stellar type is the spectra of brown dwarfs are more like red dwarf's spectra? …
questionhang's user avatar
  • 3,157
2 votes
2 answers
1k views

about H$_\alpha$ and H$_\beta$ lines in astronomical objects' spectra

Generally there may be some line ratio between the two lines. If H$\alpha$ is strong, it is quite possible we can see H$_\beta$ too. Is it possible we can see H$_\beta$, but can not see H$_\alpha$? …
questionhang's user avatar
  • 3,157
6 votes
1 answer
191 views

Clarification of radio spectrum terminology

For a radio spectrum, when is it called thermal emission, synchrotron emission, self-absorbed synchrotron emission and inverted spectrum? They are all power-law and their difference is power-law index …
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