HR4049LightCurve.png
Size of this preview:
800 × 520 pixels
.
Other resolutions:
320 × 208 pixels
|
640 × 416 pixels
|
1,024 × 666 pixels
|
1,500 × 975 pixels
.
Summary
| Description |
English:
A light curve for HR 4049. The main plot shows the V band variation over one orbital period. The inset plot shows that the amplitude of the light curve decreases at longer observing wavelengths, because the opacity of the dust decreases. Adapted from Jorissen & Frankowski (2008) DOI: 10.1063/1.2999998
|
| Date | |
| Source | Own work |
| Author | PopePompus |
Licensing
I, the copyright holder of this work, hereby publish it under the following license:
This file is licensed under the
Creative Commons
Attribution-Share Alike 4.0 International
license.
-
You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
-
Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
- share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.