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Origin of ob. Brave Tom Edward S. The Young Trawler R. Continental Monthly, Vol. Lady Luck Hugh Wiley. Compare this to the current age of the Sun at about five billion years.
The Hipparcos satellite provided measurements that located a dozen OB associations within parsecs of the Sun. These associations can be quite sparse, spanning 1, light-years in diameter.
Young stellar groups can contain a number of infant T Tauri stars that are still in the process of entering the main sequence.
These sparse populations of up to a thousand T Tauri stars are known as T associations. T associations are often found in the vicinity of the molecular cloud from which they formed.
Some, but not all, include O—B class stars. Group members have the same age and origin, the same chemical composition, and the same amplitude and direction in their vector of velocity.
Associations of stars that illuminate reflection nebulae are called R associations , a name suggested by Sidney van den Bergh after he discovered that the stars in these nebulae had a non-uniform distribution.
Because R associations are more plentiful than OB associations, they can be used to trace out the structure of the galactic spiral arms. If the remnants of a stellar association drift through the Milky Way as a somewhat coherent assemblage, then they are termed a moving group or kinematic group.
Moving groups can be old, such as the HR moving group at two billion years, or young, such as the AB Dor Moving Group at only million years.
Moving groups were studied intensely by Olin Eggen in the s. This is sufficiently close that the Sun lies in its outer fringes, without being part of the group.
The list of young moving groups is constantly evolving. The three Associations are not very distinct from each other, and have similar kinematic properties.
Young moving groups have well known ages and can help with the characterization of objects with hard to estimate ages , such as brown dwarfs.
A stellar stream is an association of stars orbiting a galaxy that was once a globular cluster or dwarf galaxy that has now been torn apart and stretched out along its orbit by tidal forces.
Some nearby kinematic groups include: . From Wikipedia, the free encyclopedia. Redirected from OB association. It is not to be confused with radial velocity , proper motion , or peculiar velocity.
See also: Galactic halo. Main article: Stellar association. See also: List of stellar streams. Star portal.
Australia Telescope Outreach and Education. Commonwealth Scientific and Industrial Research Organisation. Retrieved Annual Review of Astronomy and Astrophysics.
Astronomical Journal. Bibcode : AJ Monthly Notices of the Royal Astronomical Society. Galactic Dynamics. Princeton University Press.
Bibcode : Natur. Summary of the astrometric, photometric, and survey properties". May The Astrophysical Journal. Bibcode : ApJ Publications of the Astronomical Society of the Pacific.
Bibcode : PASP American Scientist. Pregnancy test Leopold's maneuvers Prenatal testing. Obstetric ultrasonography Nuchal scan Anomaly scan Fetal movement counting Contraction stress test Nonstress test Vibroacoustic stimulation Biophysical profile Amniotic fluid index Umbilical artery dopplers.
Chorionic villus sampling Amniocentesis Triple test Quad test Fetoscopy Fetal scalp blood testing Fetal scalp stimulation test Percutaneous umbilical cord blood sampling Apt test Kleihauer—Betke test Lung maturity Lecithin—sphingomyelin ratio Lamellar body count Fetal fibronectin test.
Fetal surgery Fetendo Podalic version External cephalic version Amnioinfusion. Artificial rupture of membranes Episiotomy Symphysiotomy Forceps in childbirth Ventouse in childbirth Odon device.
McRoberts maneuver Wood's screw maneuver Zavanelli maneuver. Manual placenta removal. Hysterectomy B-Lynch suture. Authority control NDL : Categories : Obstetrics Gynaecology.
So every time you do an echo, the output of that is added to the buffer. Trivial example: say you want to show the user an error message, but the script has already sent some HTML to the browser.
It'll look ugly, with a half-rendered page and then an error message. With Regards, Hossein. The page you are trying to view cannot be shown because it uses an invalid or unsupported form of compression.
Some web hosting servers mine do, at least have in their php. Since I spent a lot of time scouring the net searching for a work-around.
It seems to me that rewriting occurs in the very same buffering envelope where the session gets started, not at the final output stage.
Careful with while using functions that change headers of a page; that change will not be undone when ending output buffering.
If you for instance have a class that generates an image and sets the appropriate headers, they will still be in place after the end of ob.
Though the image will not be sent to the client, the png header is still in place; if you do html output here, the browser will most likely display "image error, cannot be viewed", at least firefox does.
When used in constructor part of class it have to be prefixed by "self::" or by classname, else PHP fails to create buffer.
Following clement dot ayme at st dot com 's remark : In my experience it seems that the output IS buffered, but ALSO sent to the standard output!
There is no start flag problem. One just has to notice that the second parameter is not a mode but consists of bitwise-OR'ed flags. In extension to the compress function posted below, here's a nifty little class that improves the idea a bit.
Basically, running that compress function for all your CSS for every single page load is clearly far less than optimal, especially since the styles will change only infrequently at the very worst.
The contents of each file are saved in compress 'd form in a cache file that is only recreated when the corresponding source CSS changes.
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