Difference between revisions of "BRC4"
From CoolWiki
Jump to navigationJump to searchm |
m |
||
| (One intermediate revision by the same user not shown) | |||
| Line 26: | Line 26: | ||
(Babar, you will have to do an Aladdin demo for us at some point!) | (Babar, you will have to do an Aladdin demo for us at some point!) | ||
| − | It *is* pretty, but the spitzer data just don't scream "YSOs" to me. The cloud is INSANELY bright in the MIR. I don't see a lot of point sources clearly associated with it. | + | It *is* pretty, but the spitzer data just don't scream "YSOs" to me. The cloud is INSANELY bright in the MIR (these are log scale rather than zscale, otherwise you'd just see the cloud. Seriously. I don't see a lot of point sources clearly associated with it. top to bottom, left to right, i1i2i3i4m1m2, e.g., 3.6, 4.5, 5.8, 8, 24, and 70 microns. |
[[image:brc4spitzerbands.png]] | [[image:brc4spitzerbands.png]] | ||
Latest revision as of 23:24, 26 January 2012
SIMBAD literature search shows several papers:
This one has:
- Known IRAS source associated with it.
- Known sample of YSOs?... need to read the literature a bit more.
- There is a lot of optical emission, which is likely from gas. Is this an HII region?
- But, it looks cool.
The image below is constructed using: blue = DPOSS2 (blue) green = 2MASS J red = 2MASS Ks
And the Preview image generated by Aladdin
--Ali 15:09, 25 January 2012 (PST)
(Babar, you will have to do an Aladdin demo for us at some point!)
It *is* pretty, but the spitzer data just don't scream "YSOs" to me. The cloud is INSANELY bright in the MIR (these are log scale rather than zscale, otherwise you'd just see the cloud. Seriously. I don't see a lot of point sources clearly associated with it. top to bottom, left to right, i1i2i3i4m1m2, e.g., 3.6, 4.5, 5.8, 8, 24, and 70 microns.
