Astronomy:Lockman Hole
The Lockman Hole is an area of the sky in which minimal amounts of neutral hydrogen gas are observed from the perspective of Earth. The Lockman Hole is a relatively clear window on distant objects, which makes it an attractive area of the sky for observational astronomy surveys. It is located near the pointer stars of the Big Dipper in the constellation Ursa Major and is ~15 square degrees in size.[1][2]
The Lockman Hole is named after its discoverer, astronomer F. Jay Lockman.
Location
The Lockman Hole is located at about RA 10h 45m, Dec. +58° and is defined by a region of low neutral hydrogen gas and dust column density.[3] Column density is a commonly used measure in astronomy for the quantity of a given chemical element or molecule in a certain direction. In this region, the typical column density of neutral hydrogen is NH = 0.6 x 1020 cm−2.[4] This column density is moderately lower than typical values near the galactic poles, where NH [math]\displaystyle{ \sim }[/math] 1020 cm−2, and H I column densities of NH > 1021 cm−2 are common at low galactic latitudes and towards H I clouds.[5]
The region around B1950.0 RA 10h 45m Dec 57° 20′ has a minimum NH of 4.5 x 1019 cm−2.[3] There is a diffuse cloud covering half of the field.[3][6]
The Lockman Hole East is a subregion of the Lockman Hole centered at J2000.0 RA 10h 52m Dec +57°.[7]
The Lockman Hole North-west (LHNW) is a region that appears about as wide as the moon centered at J2000.0 RA 10h 34m Dec +57° 40′.,[8][9] with a column density of NH = 5.72 x 1019 cm−2.[5]
Hydrogen gas absorption and emission
Clouds of neutral hydrogen are ubiquitous in the Milky Way galaxy, and effectively absorb photons that are energetic enough to ionize hydrogen, which requires an energy of 13.6 electron volts (in the extreme ultraviolet range). Even the relatively small amounts of hydrogen in the Lockman Hole absorb most radiation at and just above energies of 13.6 electron volts, but even so it transmits extreme ultraviolet and soft x-ray radiation from extragalactic objects to a greater degree than other areas of the sky.
Neutral hydrogen is also associated with diffuse emission at infrared wavelengths that can confuse observations of faint infrared sources.
Observations
The relatively clear field of view offered by the Lockman Hole has allowed its use to view extremely distant regions of the universe. Observations by the Spectral and Photometric Imaging Receiver (SPIRE) instrument aboard the Herschel Space Telescope of the Lockman Hole have imaged thousands of extremely distant galaxies that appear as they did 10–12 billion years ago.[10]
This field of view also contains hundreds of astronomical X-ray sources, some of them supermassive black holes. The Chandra X-ray Observatory and ROSAT have been used to study X-ray sources from the Lockman Hole.[4] Some 75 X-ray sources are observed with the PSPC of ROSAT.[4]
Detailed X-ray spectral analysis has been performed on 123 X-ray sources in the Lockman Hole using XMM-Newton.[11]
The diffuse X-ray background (XRB) has also been studied in the area.[12][13]
Active galactic nuclei have also been studied in the area, for example MBC2005.[11]
See also
- Chandra Deep Field South - a similar clear field-of-view
- Interstellar medium
- Local Bubble
- Local Interstellar Cloud
References
- ↑ "Is the Big Dipper scooping dark matter?". CSMonitor.com. 2011-02-18. http://www.csmonitor.com/Science/2011/0218/Is-the-Big-Dipper-scooping-dark-matter.
- ↑ "Lockman Hole". Encyclopedia of Science. http://www.daviddarling.info/encyclopedia/L/Lockman_Hole.html. Retrieved 2011-12-10.
- ↑ 3.0 3.1 3.2 "The structure of galactic HI in directions of low total column density". Astrophys. J. 302 (3): 432–49. Mar 1986. doi:10.1086/164002. Bibcode: 1986ApJ...302..432L.
- ↑ 4.0 4.1 4.2 Hasinger G, Burg R, Giacconi R, Hartner G, Schmidt M, Trumper J, Zamorani G; Burg; Giacconi; Hartner; Schmidt; Trumper; Zamorani (Aug 1993). "A Deep X-Ray Survey in the Lockman-Hole and the Soft X-Ray N-Log". Astron. Astrophys. 275 (1): 1–15. Bibcode: 1993A&A...275....1H.
- ↑ 5.0 5.1 "H I in the Galaxy". Annu. Rev. Astron. Astrophys. 28 (1): 215–61. 1990. doi:10.1146/annurev.aa.28.090190.001243. Bibcode: 1990ARA&A..28..215D.
- ↑ "Maps of dust infrared emission for use in estimation of reddening and cosmic microwave background radiation foregrounds". Astrophys. J. 500 (2): 525–53. Jun 1998. doi:10.1086/305772. Bibcode: 1998ApJ...500..525S.
- ↑ "SHADES: SCUBA Half Degree Extragalactic Survey". http://www.roe.ac.uk/ifa/shades/maps.html.
- ↑ "Shape of Universe seen during adolescent years". Spaceflight Now. 2003-03-23. http://www.spaceflightnow.com/news/n0303/28chandra/.
- ↑ "The Chandra Large Area Synoptic X-Ray Survey (CLASXS) of the Lockman Hole-Northwest: The X-Ray Catalog". Astron. J. 128 (4): 1501–23. Oct 2004. doi:10.1086/423996. Bibcode: 2004AJ....128.1501Y.
- ↑ "Star-forming galaxies like grains of sand". http://oshi.esa.int/#detail=image.html?id=36.
- ↑ 11.0 11.1 "XMM-Newton observations of the Lockman Hole: search for AGNs". Astron. Astrophys. 444 (1): 79–99. Dec 2005. doi:10.1051/0004-6361:20052881. Bibcode: 2005A&A...444...79M.
- ↑ Mather, J. C.; Cheng, E. S.; Cottingham, D. A.; Eplee, R. E., Jr.; Fixsen, D. J.; Hewagama, T.; Isaacman, R. B.; Jensen, K. A. et al. (January 1994). "Measurement of the cosmic microwave background spectrum by the COBE FIRAS instrument". The Astrophysical Journal 420 (2): 439–44. doi:10.1086/173574. Bibcode: 1994ApJ...420..439M.
- ↑ Mather et al. (1990). "A preliminary measurement of the cosmic microwave background spectrum by the Cosmic Background Explorer (COBE) satellite". Astrophys. J. 354: L37. doi:10.1086/185717. Bibcode: 1990ApJ...354L..37M.
Further reading
- "The structure of galactic HI in directions of low total column density". Astrophys. J. 302 (3): 432–49. Mar 1986. doi:10.1086/164002. Bibcode: 1986ApJ...302..432L.
External links
- Lockman Hole at Chandra
- Animations of Lockman Hole
- The Lockman Hole by the Herschel Space Observatory
- Spitzer Space Telescope and the Lockman Hole
- XMM-Newton Observations of the Lockman Hole
- The Lockman Hole from the Max-Planck-Institut für extraterrestrische Physik
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