Perseus molecular cloud
{{Short description|Region in the constellation of Perseus}}
{{no footnotes|date=March 2021}}
{{infobox nebula
|name= Perseus Molecular Cloud
|image= PerseusCloudMap.png
|caption= Map of the Perseus molecular cloud
|type= giant molecular cloud
|epoch= J2000.0{{cite simbad |title= NAME Perseus Cloud |accessdate= 2014-03-14 }}
|constellation= Perseus
|dist_ly= 956–1047
|size_v= 6°×2°
|names= Perseus Molecular Cloud, Perseus Cloud, Per MCld, Per Mol Cloud, Perseus Complex, PMC
}}
The Perseus molecular cloud (Per MCld) is a nearby (~1000 ly) giant molecular cloud in the constellation of Perseus and contains over 10,000 solar masses of gas and dust covering an area of 6 by 2 degrees. Unlike the Orion molecular cloud it is almost invisible apart from two clusters, IC 348 and NGC 1333, where low-mass stars are formed. It is very bright at mid and far-infrared wavelengths and in the submillimeter originating in dust heated by the newly formed low-mass stars.
It shows a curious ring structure in maps made by the IRAS and MSX satellites and the Spitzer Space Telescope and has been detected by the COSMOSOMAS at microwave frequencies as a source of anomalous "spinning dust" emission.
{{multipleimage |header=Perseus Molecular Cloud |align=center | caption_align=center |direction=vertical |width= |image1=PIA23405-PerseusMolecularCloud-SkyLocation.jpg |caption1=Location |width1=500 |image2=PIA23405-PerseusMolecularCloud-Annotated.jpg |caption2=Annotated |width2=500 |image3=PIA23405-PerseusMolecularCloud-FullRez.jpg |caption3=Full resolution |width3=500 |footer=Spitzer Space Telescope (19 December 2019) }}
References
{{reflist}}
- {{cite book|author=Bally, J.|author2=Walawender, J.|author3=Johnstone, D.|author4=Kirk, H.|author5=Goodman, A.|title=The Perseus Cloud|bibcode=2008hsf1.book..308B|journal=Handbook of Star Forming Regions, Volume I: The Northern Sky ASP Monograph Publications|volume=4|page=308|date=December 2008|isbn=978-1-58381-670-7}}
- {{cite journal|author=Kirk, Helen|author2=Johnstone, Doug|author3=Di Francesco, James|title=The Large- and Small-Scale Structures of Dust in the Star-forming Perseus Molecular Cloud|bibcode=2006ApJ...646.1009K|journal=The Astrophysical Journal|volume=646|issue=2|pages=1009–1023|date=August 2006|doi=10.1086/503193|arxiv = astro-ph/0602089 |s2cid=1173412 }}
- More on THE ASTROPHYSICAL JOURNAL http://iopscience.iop.org/0004-637X/656/1/293
{{DEFAULTSORT:Perseus Molecular Cloud}}