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Dense stellar wind
A superwind is an extremely dense wind emanating from asymptotic giant branch (AGB) stars towards the end of their lives. While the exact origin of the
Superwind
Strong stellar winds of a galactic scale in size
A galactic superwind, or just galactic wind, is a high velocity stellar wind emanating from either newly formed massive stars, spiral density waves, or
Galactic_superwind
Galaxy in the constellation Canes Venatici
the plane of the galaxy. This superwind can be seen in X-rays and in spectral line emission. The gas from this superwind has produced a giant, diffuse
NGC_4631
Odd radio circle in the constellation Canes Venatici
black hole mergers, or powerful superwinds. Recent theoretical work proposes that the rings may be linked to superwind outflows from spiral host radio
RAD_J131346.9+500320
Spiral galaxy in the constellation Virgo
47–90. ISSN 0365-0138. "The Superwind Galaxy". ESO. 1 September 2010. "Extra-planar Hot Gas and Magnetic Fields in the Superwind Galaxy NGC 4666". ESA. 24
NGC_4666
Flow of gas ejected from the upper atmosphere of a star
Planetary wind Colliding-wind binary Pulsar wind nebula Galactic superwind Superwind Planetary nebula Asymptotic giant branch Lamers, Henny J. G. L. M
Stellar_wind
Cavity of hot gas blown from a star
Planetary wind Colliding-wind binary Pulsar wind nebula Galactic superwind Superwind Castor, J.; McCray, R.; Weaver, R. (1975). "Interstellar Bubbles"
Stellar-wind_bubble
Nebula powered by the pulsar wind of a pulsar
Planetary wind Stellar-wind bubble Colliding-wind binary Galactic superwind Superwind Orders of magnitude (magnetic field) Weiler, K. W.; Panagia, N. (November
Pulsar_wind_nebula
Spiral with constant distance from itself
Naomi; Hsieh, I-Ta (March 2017). "The large-scale nebular pattern of a superwind binary in an eccentric orbit". Nature Astronomy. 1 (3): 0060. arXiv:1704
Archimedean_spiral
Binary star system in which two massive stars emit powerful stellar winds
wind Planetary wind Stellar-wind bubble Pulsar wind nebula Galactic superwind Superwind Volpi, Delia; Blomme, Ronny; De Becker, Michael; Rauw, Gregor (December
Colliding-wind_binary
Galaxy in the constellation Ursa Major
starburst clusters from our vantage point. M82's unique bipolar outflow (or 'superwind') appears to be concentrated on clumps A and C, and is fueled by energy
Messier_82
Nuclear fusion reaction
stellar wind driven by radiation pressure, which ultimately becomes a superwind as the star enters the planetary nebula phase. The triple-alpha process
Triple-alpha_process
Galaxy in the constellation of Pavo
kinematics, strongly suggest that NGC 6810 is host to a galactic-scale superwind which is streaming from the starburst region. The actively star-forming
NGC_6810
Japanese-American meteorologist (1920–1998)
comparatively little damage. "Wind expert says Andrew generated small superwinds". United Press International. Tampa, Florida. 20 May 1993. Retrieved 15
Ted_Fujita
Constellation in the northern sky
presence of a supermassive black hole. The structure itself is formed by superwinds from the black hole. NGC 3310 is another starburst spiral galaxy located
Ursa_Major
Cosmic stream of charged particles
weight. Galactic superwind Stellar wind Solar wind Planetary wind Stellar-wind bubble Colliding-wind binary Pulsar wind nebula Superwind Shelton, Jim (July
Cosmic_wind
Changes to stars over their lifespans
contract again, going through a period of post-asymptotic-giant-branch superwind to produce a planetary nebula with an extremely hot central star. The
Stellar_evolution
Intermediate spiral galaxy in the constellation Sculptor
supernovae have blown out material to NGC 253's halo in the form of a superwind that seems to be inhibiting star formation in the galaxy. Although supernovae
Sculptor_Galaxy
tens of solar masses. The lost mass is expected to have been expelled by superwinds: high velocity winds that are driven by the hot photosphere into interstellar
List_of_most_massive_stars
Stage of stellar evolution
regularly, occurs after fusion has ceased and the star has entered the superwind phase. These stars are "born again" with unusual properties. Despite the
Horizontal_branch
Red Supergiant Star in Open Cluster Stephenson 2
alone, suggesting possible additional mechanisms such as a short-lived superwind phase or multiple star interactions and the star is a progenitor for a
Stephenson_2_DFK_52
Low-redshift quasar and galaxy merger in the constellation Boötes
photoionization or shocked emission via a quasar-driven superwind. A study also mentions the superwind driven by the quasar is prototypical. SDSS J135646.10+102609
SDSS_J135646.10+102609.0
Radio galaxy in the constellation Virgo
AGN's anisotropic hard radiation. Alternatively, it might be created by superwind outflows, given the galaxy showed elongated core-like or bubble structures
4C_03.24
Galaxy in the constellation Virgo
ago. Multiple supernovae (up to 100,000) in the nucleus have produced 'superwinds' that are blowing the galaxy's interstellar medium outward into the intracluster
Messier_90
Galaxy in the constellation Lynx
is associated with it. The vigorous star formation creates an unusual "superwind" of out-flowing gas, which has been detected in X-rays as a bubble like
NGC_2782
Cool giant star with approximately equal quantities of carbon and oxygen in its atmosphere
form a visible detached shell. The shells are thought to form during a superwind phase very late in the AGB evolution. BD Camelopardalis is a naked-eye
S-type_star
Galaxy in the constellation Vela
ionised gas from the northern nucleus with shocks which is attributed to a superwind powered by the starburst. Based on observations by Spitzer Space Telescope
NGC_3256
Galaxy in the constellation Ursa Major
NGC 3079. HST: Burst of Star Formation Drives Bubble in Galaxy's Core Superwind Sculpts Filamentary Features - Chandra X-ray Observatory NASA Astronomy
NGC_3079
Galaxy in the constellation Camelopardalis
might be numerous and commonplace. A study named: "Dense CO in Mrk 71-A: Superwind Suppressed in a Young Super Star Cluster" was published in the Astrophysical
NGC_2366
Radio galaxy in the constellation Draco
galactic nucleus host shows Lyα emission that indicative of a galaxy-wide "superwind". Moreover, the host is found to have a luminous highly ionized outflow
4C_+72.26
Possible type of luminous blue compact galaxy
Green Peas: Suppressed Superwinds in Candidate LyC Emitters". Within the paper, they say that current thinking describes how superwinds clear neutral gas away
Pea_galaxy
Galaxy in the constellation Columba
Dragan; et al. (November 2017). "Evolution of Molecular Clouds in the Superwind Galaxy NGC 1808 Probed by ALMA Observations". The Astrophysical Journal
NGC_1808
British astrophysicist (1951–2012)
discovery of the first, X-ray selected BL Lac object, discovery of the first "superwind" galaxy, and discovery of strong magnetic fields in the jets of young
David_Axon
Galaxy in the constellation Sextans
spectrum of the type II-L supernova 1984E in NGC 3169 Further evidence for a superwind?", Publications of the Astronomical Society of the Pacific, 99: 112–115
NGC_3169
Quasar in the constellation Pegasus
Pece; Wilkes, Belinda; Haas, Martin (2017-06-01). "Starburst-driven Superwinds in Quasar Host Galaxies". The Astrophysical Journal Letters. 843 (1):
3C_432
Galaxy in the constellation of Cetus
Kewley, L. J.; Rupke, D. S. N. (2010). "NGC 839: Shocks in an M82-like Superwind". The Astrophysical Journal. 721 (1): 505–517. arXiv:1007.3495. Bibcode:2010ApJ
NGC_839
Spiral galaxy in the constellation Leo
which suggest that the spurs originated in a starburst superbubble or superwind. The northern part of an Hα nebula of NGC 3859 seems to be flowing toward
NGC_3859
Interstellar clouds
Alan (2009-01-01). "Extended Emission-Line Regions: Remnants of Quasar Superwinds?". The Astrophysical Journal. 690 (1): 953–973. arXiv:0809.1117. Bibcode:2009ApJ
Extended_emission-line_region
American astronomer
evolution Kinematic feedback: Supernova-driven superbubbles and galactic superwinds Massive star and clusters Finding no star bigger than 200 solar masses
Sally_Oey
Galaxy in the constellation Pavo
Lipari, Sebastian; Macchetto, F. (1991-09-01). "Massive Star Formation and Superwinds in IRAS 19254-7245 (The Superantennae)". The Astrophysical Journal. 379:
IRAS_19254−7245
Fujita". Storm Track. 22 (1). "Wind expert says Andrew generated small superwinds". United Press International. Tampa, Florida. 20 May 1993. Retrieved 15
List_of_tornadic_researchers
Quasar in the constellation Orion
Podigachoski, Pece; Wilkes, Belinda; Haas, Martin (2017). "Starburst-driven Superwinds in Quasar Host Galaxies". The Astrophysical Journal Letters. 843 (1):
4C_+09.17
Canadian-German astronomer
galaxies in the early universe, and investigated the effects of galactic superwinds on star formation. Her contributions also include work on the instrumentation
Natascha_Förster_Schreiber
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Female
English
Variant spelling of English Ailsa, AILSIE means "elf victory."
Boy/Male
Hindu
Prepared
Boy/Male
Assamese, Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Sanskrit, Tamil
Truth; Faithful; God; Final Truth of Universe; Who Speaks Truth
Boy/Male
Indian, Tamil
Satisfaction
Boy/Male
Teutonic
Nation's army.
Girl/Female
Tamil
Mriganayani | மரகநயநீ
Doe eyed
Boy/Male
Australian, Biblical, Christian, Danish, French, Hebrew
Son of My Sorrow or Pain; Son of My Sorrows
Boy/Male
Bengali, Indian
Know Yourself
Male
English
Short form of English Timothy, TIM means "to honor God."
Boy/Male
French, Hebrew, Hindu, Indian
Wolf; A Prince
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