Just a sample of the Echomail archive
ESSNASA:
[ << oldest | < older | list | newer > | newest >> ]
|  Message 9,056 of 10,785  |
|  Alan Ianson to All  |
|  Daily APOD Report  |
|  25 Jul 23 05:55:12  |
 
MSGID: 1:153/757.0 44da8f6f
TZUTC: -0700
CHRS: LATIN-1 2
Astronomy Picture of the Day
Discover the cosmos! Each day a different image or photograph of our
fascinating universe is featured, along with a brief explanation
written by a professional astronomer.
2023 July 25
Pillars of gas and dark dust extend diagonally from the bottom left to
the upper right. Bright X-ray sources are superimposed as bright dots
around the image. Infrared dust glows behind the pillars. Please see
the explanation for more detailed information.
The Eagle Nebula with X-ray Hot Stars
Image Credit: X-ray: Chandra: NASA/CXC/SAO, XMM: ESA/XMM-Newton; IR:
JWST: NASA/ESA/CSA/STScI, Spitzer: NASA/JPL/CalTech; Visible: Hubble:
NASA/ESA/STScI, ESO; Image Processing: L. Frattare, J. Major, N. Wolk,
and K. Arcand
Explanation: What do the famous Eagle Nebula star pillars look like in
X-ray light? To find out, NASA's orbiting Chandra X-ray Observatory
peered in and through these interstellar mountains of star formation.
It was found that in M16 the dust pillars themselves do not emit many
X-rays, but a lot of small-but-bright X-ray sources became evident.
These sources are shown as bright dots on the featured image which is a
composite of exposures from Chandra (X-rays), XMM (X-rays), JWST
(infrared), Spitzer (infrared), Hubble (visible), and the VLT
(visible). What stars produce these X-rays remains a topic of research,
but some are hypothesized to be hot, recently-formed, low-mass stars,
while others are thought to be hot, older, high-mass stars. These X-ray
hot stars are scattered around the frame -- the previously identified
Evaporating Gaseous Globules (EGGS) seen in visible light are not
currently hot enough to emit X-rays.
Tomorrow's picture: undersea overhead
__________________________________________________________________
Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)
NASA Official: Phillip Newman Specific rights apply.
NASA Web Privacy Policy and Important Notices
A service of: ASD at NASA / GSFC,
NASA Science Activation
& Michigan Tech. U.
--- BBBS/Li6 v4.10 Toy-6
* Origin: The Rusty MailBox - Penticton, BC Canada (1:153/757)
SEEN-BY: 1/123 10/0 1 15/0 90/1 92/1 102/401 103/1 17 705 105/81 106/201
SEEN-BY: 123/131 129/305 134/100 153/135 143 757 802 6809 7715 214/22
SEEN-BY: 218/0 1 215 700 810 840 850 860 880 900 221/1 6 226/30 227/114
SEEN-BY: 229/110 112 113 206 307 317 400 426 428 470 664 700 240/1120
SEEN-BY: 266/512 282/1038 291/111 301/1 113 812 317/3 320/219 322/757
SEEN-BY: 335/364 341/66 342/200 396/45 460/58 633/280 712/848 5020/400
SEEN-BY: 5020/1042 5075/35
PATH: 153/757 221/6 301/1 218/700 229/426
|
[ << oldest | < older | list | newer > | newest >> ]
(c) 1994, bbs@darkrealms.ca