Matches in SemOpenAlex for { <https://semopenalex.org/work/W3104324770> ?p ?o ?g. }
- W3104324770 endingPage "35" @default.
- W3104324770 startingPage "35" @default.
- W3104324770 abstract "Near-infrared imaging polarimetry in the J, H, and Ks bands has been carried out for the protostellar cluster region around NGC 2264 IRS 2 in the Monoceros OB1 molecular cloud. Various infrared reflection nebula clusters (IRNCs) associated with NGC 2264 IRS 2 and the IRAS 12 S1 core, as well as local infrared reflection nebulae (IRNe), were detected. The illuminating sources of the IRNe were identified with known or new near- and mid-infrared sources. In addition, 314 point-like sources were detected in all three bands and their aperture polarimetry was studied. Using a color–color diagram, reddened field stars and diskless pre-main-sequence stars were selected to trace the magnetic field (MF) structure of the molecular cloud. The mean polarization position angle of the point-like sources is 81° ± 29° in the cluster core, and 58° ± 24° in the perimeter of the cluster core, which is interpreted as the projected direction on the sky of the MF in the observed region of the cloud. The Chandrasekhar–Fermi method gives a rough estimate of the MF strength to be about 100 μG. A comparison with recent numerical simulations of the cluster formation implies that the cloud dynamics is controlled by the relatively strong MF. The local MF direction is well associated with that of CO outflow for IRAS 12 S1 and consistent with that inferred from submillimeter polarimetry. In contrast, the local MF direction runs roughly perpendicular to the Galactic MF direction." @default.
- W3104324770 created "2020-11-23" @default.
- W3104324770 creator A5012939955 @default.
- W3104324770 creator A5013556814 @default.
- W3104324770 creator A5017309702 @default.
- W3104324770 creator A5022831412 @default.
- W3104324770 creator A5024214300 @default.
- W3104324770 creator A5024765355 @default.
- W3104324770 creator A5039113915 @default.
- W3104324770 creator A5046107590 @default.
- W3104324770 creator A5068596635 @default.
- W3104324770 creator A5072082931 @default.
- W3104324770 creator A5079883757 @default.
- W3104324770 creator A5081451517 @default.
- W3104324770 date "2011-10-13" @default.
- W3104324770 modified "2023-10-17" @default.
- W3104324770 title "COMPLEX SCATTERED RADIATION FIELDS AND MULTIPLE MAGNETIC FIELDS IN THE PROTOSTELLAR CLUSTER IN NGC 2264" @default.
- W3104324770 cites W1559614313 @default.
- W3104324770 cites W1615124923 @default.
- W3104324770 cites W1619205399 @default.
- W3104324770 cites W1963655933 @default.
- W3104324770 cites W1964299149 @default.
- W3104324770 cites W1967057627 @default.
- W3104324770 cites W1969297889 @default.
- W3104324770 cites W1969392028 @default.
- W3104324770 cites W1974671582 @default.
- W3104324770 cites W1975014135 @default.
- W3104324770 cites W1981241669 @default.
- W3104324770 cites W1981808693 @default.
- W3104324770 cites W1982500251 @default.
- W3104324770 cites W1982609704 @default.
- W3104324770 cites W1984544315 @default.
- W3104324770 cites W1985163476 @default.
- W3104324770 cites W1990670394 @default.
- W3104324770 cites W1990913428 @default.
- W3104324770 cites W1991481107 @default.
- W3104324770 cites W1994188280 @default.
- W3104324770 cites W1994857665 @default.
- W3104324770 cites W1995104333 @default.
- W3104324770 cites W1995362031 @default.
- W3104324770 cites W1997731820 @default.
- W3104324770 cites W1998644240 @default.
- W3104324770 cites W1998712918 @default.
- W3104324770 cites W2000495860 @default.
- W3104324770 cites W2003766068 @default.
- W3104324770 cites W2004024124 @default.
- W3104324770 cites W2004741935 @default.
- W3104324770 cites W2006503284 @default.
- W3104324770 cites W2008067559 @default.
- W3104324770 cites W2010023165 @default.
- W3104324770 cites W2012161777 @default.
- W3104324770 cites W2012547924 @default.
- W3104324770 cites W2016771645 @default.
- W3104324770 cites W2019440065 @default.
- W3104324770 cites W2019557778 @default.
- W3104324770 cites W2020298240 @default.
- W3104324770 cites W2020863449 @default.
- W3104324770 cites W2021030726 @default.
- W3104324770 cites W2022429968 @default.
- W3104324770 cites W2024126458 @default.
- W3104324770 cites W2024425170 @default.
- W3104324770 cites W2024500648 @default.
- W3104324770 cites W2024608061 @default.
- W3104324770 cites W2026670653 @default.
- W3104324770 cites W2026795906 @default.
- W3104324770 cites W2026911454 @default.
- W3104324770 cites W2028109099 @default.
- W3104324770 cites W2028928164 @default.
- W3104324770 cites W2035044321 @default.
- W3104324770 cites W2040140712 @default.
- W3104324770 cites W2041867338 @default.
- W3104324770 cites W2042337148 @default.
- W3104324770 cites W2045604928 @default.
- W3104324770 cites W2049427488 @default.
- W3104324770 cites W2051401790 @default.
- W3104324770 cites W2056400752 @default.
- W3104324770 cites W2057122781 @default.
- W3104324770 cites W2058837045 @default.
- W3104324770 cites W2059686127 @default.
- W3104324770 cites W2065643668 @default.
- W3104324770 cites W2066151326 @default.
- W3104324770 cites W2068044333 @default.
- W3104324770 cites W2068475862 @default.
- W3104324770 cites W2069648054 @default.
- W3104324770 cites W2072159034 @default.
- W3104324770 cites W2075201246 @default.
- W3104324770 cites W2075723338 @default.
- W3104324770 cites W2078834481 @default.
- W3104324770 cites W2078923655 @default.
- W3104324770 cites W2082877321 @default.
- W3104324770 cites W2083647828 @default.
- W3104324770 cites W2083892838 @default.
- W3104324770 cites W2088201186 @default.
- W3104324770 cites W2088773507 @default.
- W3104324770 cites W2092575992 @default.
- W3104324770 cites W2094092391 @default.
- W3104324770 cites W2098170381 @default.
- W3104324770 cites W2129278855 @default.