(2.491 × 2.341 piksel, fayl həcmi: 4,59 MB, MIME növü: image/png)

Bu fayl Vikianbardandır və digər
layihələrdə istifadə edilə bilər.
təsvir səhifəsi
təsvir səhifəsi
Faylın təsvir səhifəsinə get

Xülasə

İzah

There are two reasons why this galaxy is interesting aside from the fact that it is one of those neat, geometric lenticular galaxies. First, as a Seyfert I type, it has an active nucleus. Rick Edelson has an easy to read article on that aspect and its variability . If you want something harder to read, you might try by T. J. Turner et al, which I think also mentions the second interesting thing which is easily seen in this picture. There are some blue clouds of gas to go along with those darker strands of dust near the nucleus.

I've learned that if you see something glowing blue in space, it's probably doing that because of ionization. Given the crazy amounts of energy being output by the active nucleus, it's not surprising that it happens, but I admit that it seems crazy that it is able to have this effect reach so far out from it. Anyway, I don't understand it very well, so take my explanation with a grain of salt.

Smallish dots of light scattered around I presume to be globular clusters associated with the galaxy. They are conspicuous given how otherwise smooth the galaxy appears.

Note that though the blue clouds were only visible in the blue channel (F450W) they appear bright and almost white in my image. I did this to make them easier to discern. Anytime something is present only in the blue channel it tends to get lost against the background.

Another thing to note is that I aggressively sharpened the dust and these blue features. They are easy to see in reality but increasing their contrast allows us to see the fainter parts much more easily.

Furthermore, only the center of this image is in color as the nucleus was imaged in 1998 by Hubble's WFPC2 as part of . Later on, the whole galaxy was captured by Hubble's WFC3/UVIS instrument in a subsequent study to . Combining these two datasets, color can be generated for the center and the whole galaxy structure can be included in black and white which is ok because there really is not a lot of color away from the nucleus, anyway.

Red: hst_06633_07_wfpc2_f814w_pc_sci Green: WFC3 / UVIS F547M (ib5e02010_drz) Blue: hst_06633_07_wfpc2_f450w_pc_sci

North is up.
Tarix
Mənbə
Müəllif from Fresh Meadows, NY, USA

Lisenziya

w:az:Creative Commons
İstinad vermək
Bu fayl Creative Commons lisenziyası altında yayımlanır.
Siz heç bir məhdudiyyət olmadan:
  • paylaşa bilərsiniz – əsəri köçürə, paylaya və ötürə bilərsiniz
  • remiks edə bilərsiniz – əsəri adaptasiya edə bilərsiniz
Aşağıdakı şərtlərə əməl etməklə:
  • İstinad vermək – Müvafiq istinad verməli, lisenziyaya keçid əlavə etməli və dəyişikliklər edilib-edilmədiyini bildirməlisiniz . Siz bunu istənilən şəkildə edə bilərsiniz, lakin lisenziya verənin sizə şəxsən icazə verdiyini göstərən formada yox.
This image was originally posted to Flickr by geckzilla at . It was reviewed on 17 sentyabr 2014 by FlickreviewR and was confirmed to be licensed under the terms of the cc-by-2.0.

17 sentyabr 2014

Captions

Add a one-line explanation of what this file represents

Items portrayed in this file

təsvir edir

some value

URL:
Flickr user ID ingilis:
müəllifin qısa adı: Judy Schmidt

copyrighted ingilis

14 sentyabr 2014

media type ingilis

image/png

Faylın tarixçəsi

Faylın əvvəlki versiyasını görmək üçün gün/tarix bölməsindəki tarixlərə klikləyin.

Tarix/Vaxt Miniatür Ölçülər İstifadəçi Şərh
hal-hazırkı 2.491 × 2.341 (4,59 MB) {{Information |Description=There are two reasons why this galaxy is interesting aside from the fact that it is one of those neat, geometric lenticular galaxies. First, as a Seyfert I type, it has an active nucleus. Rick Edelson has an easy to read arti...

Aşağıdakı səhifə bu faylı istifadə edir:

Faylın qlobal istifadəsi

Bu fayl aşağıdakı vikilərdə istifadə olunur:

Metaməlumatlar


Informasiya Melumat Axtar

Anarim.Az

Sayt Rehberliyi ile Elaqe

Saytdan Istifade Qaydalari

Anarim.Az 2004-2023