File:Comparative_supernova_type_light_curves.png
From Wikipedia, the free encyclopedia
Size of this preview: 800 × 518 pixels. Other resolutions: 320 × 207 pixels | 640 × 414 pixels | 1,024 × 663 pixels | 1,187 × 768 pixels.
Original file (1,187 × 768 pixels, file size: 137 KB, MIME type: image/png)
This is a file from the Wikimedia Commons. Information from its description page there is shown below. Commons is a freely licensed media file repository. You can help. |
Summary
DescriptionComparative supernova type light curves.png |
English: This image shows light curves of the main supernova types, representative of peak brightness, rise times, and decay times. See Karttunen et al. for types Ia, Ib, II-L and II-P;[1] Modjaz et al. for types Ic and IIb;[2] and Nyholm et al. for type IIn.[3]
Русский: Кривые блеска сверхновых различных типов. |
Date | |
Source | OOCalc chart |
Author | Lithopsian |
This graph image could be re-created using vector graphics as an SVG file. This has several advantages; see Commons:Media for cleanup for more information. If an SVG form of this image is available, please upload it and afterwards replace this template with
{{vector version available|new image name}} .
It is recommended to name the SVG file “Comparative supernova type light curves.svg”—then the template Vector version available (or Vva) does not need the new image name parameter. |
Licensing
I, the copyright holder of this work, hereby publish it under the following licenses:
Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported 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.
You may select the license of your choice.
- ↑ (2016) Fundamental Astronomy, Springer, p. 309 ISBN: 978-3-662-53044-3.
- ↑ (August 2019). "New regimes in the observation of core-collapse supernovae". Nature Astronomy 3 (8): 717–724. DOI:10.1038/s41550-019-0856-2.
- ↑ (2020). "Type IIn supernova light-curve properties measured from an untargeted survey sample". Astronomy and Astrophysics 637: A73. DOI:10.1051/0004-6361/201936097.
Items portrayed in this file
depicts
4 June 2012
image/png
0d9597f8bab564b2b54c9f1db940c4f7bbecea93
140,342 byte
768 pixel
1,187 pixel
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 15:53, 4 June 2012 | 1,187 × 768 (137 KB) | Lithopsian | {{subst:Upload marker added by en.wp UW}} {{Information |Description = {{en|This image shows light curves of the main supernova types, representative of peak brightness, rise times, and decay times.}} |Source = OOCalc chart |Date = 2012-06-04 |Author =... |
File usage
The following pages on the English Wikipedia use this file (pages on other projects are not listed):
Global file usage
The following other wikis use this file:
- Usage on et.wikipedia.org
- Usage on eu.wikipedia.org
- Usage on fa.wikipedia.org
- Usage on it.wikipedia.org
- Usage on ja.wikipedia.org
- Usage on ko.wikipedia.org
- Usage on mk.wikipedia.org
- Usage on nl.wikipedia.org
- Usage on pt.wikipedia.org
- Usage on sk.wikipedia.org
- Usage on vi.wikipedia.org