Matches in SemOpenAlex for { <https://semopenalex.org/work/W3215487907> ?p ?o ?g. }
- W3215487907 endingPage "610" @default.
- W3215487907 startingPage "593" @default.
- W3215487907 abstract "Atomic ionised regions with strong continuum emission are often associated with regions of high-mass star formation and low-frequency (<2GHz) observations of these regions are needed to help build star formation models. The region toward the Vela Supernova Remnant is particularly interesting as it is a complex structure of recent supernova explosions and molecular clouds containing a number of HII regions that are not well characterised. We searched publicly available catalogues for HII regions, both candidate and identified, which also have low-frequency emission. In the area of ~400 square degrees toward the Vela Supernova remnant, we found 10 such HII regions, some of which have multiple components in catalogues. In this work we use data from the Australian Square Kilometre Array Pathfinder and previously unpublished data from the Murchison Widefield Array and the Australian Telescope Compact Array to analyse these sources. The high-mass star forming region RCW 38, with observations specifically targeted on the source, is used as a pilot study to demonstrate how low-frequency, wide-field continuum observations can identify and study HII regions in our Galaxy. For the 9 other HII regions, we discuss their properties; including information about which clouds are interacting, their ages, whether they are dominated by infrared or optical H$alpha$ lines, distances, ionising photon flux, and upper limits on the infrared luminosity. In future work, these 9 regions will be analysed in more detail, similar to the result for RCW 38 presented here." @default.
- W3215487907 created "2021-12-06" @default.
- W3215487907 creator A5018196107 @default.
- W3215487907 creator A5031837870 @default.
- W3215487907 creator A5035126916 @default.
- W3215487907 creator A5052534067 @default.
- W3215487907 creator A5085640875 @default.
- W3215487907 creator A5088366848 @default.
- W3215487907 date "2021-11-27" @default.
- W3215487907 modified "2023-10-06" @default.
- W3215487907 title "A low-frequency pilot survey of southern H <scp>ii</scp> regions in the vela constellation" @default.
- W3215487907 cites W1564915826 @default.
- W3215487907 cites W1835573494 @default.
- W3215487907 cites W1967268878 @default.
- W3215487907 cites W1969747332 @default.
- W3215487907 cites W1981309478 @default.
- W3215487907 cites W1990790296 @default.
- W3215487907 cites W1990841834 @default.
- W3215487907 cites W2001956246 @default.
- W3215487907 cites W2011301426 @default.
- W3215487907 cites W2014904361 @default.
- W3215487907 cites W2024630900 @default.
- W3215487907 cites W2025969090 @default.
- W3215487907 cites W2026755197 @default.
- W3215487907 cites W2029623000 @default.
- W3215487907 cites W2053326823 @default.
- W3215487907 cites W2055764299 @default.
- W3215487907 cites W2055881397 @default.
- W3215487907 cites W2056710613 @default.
- W3215487907 cites W2059531229 @default.
- W3215487907 cites W2066361364 @default.
- W3215487907 cites W2066658404 @default.
- W3215487907 cites W2070139809 @default.
- W3215487907 cites W2073938066 @default.
- W3215487907 cites W2082153584 @default.
- W3215487907 cites W2091123728 @default.
- W3215487907 cites W2096875730 @default.
- W3215487907 cites W2110114082 @default.
- W3215487907 cites W2116362607 @default.
- W3215487907 cites W2116790661 @default.
- W3215487907 cites W2121359722 @default.
- W3215487907 cites W2122468651 @default.
- W3215487907 cites W2135625048 @default.
- W3215487907 cites W2137122064 @default.
- W3215487907 cites W2143192129 @default.
- W3215487907 cites W2143203124 @default.
- W3215487907 cites W2150049924 @default.
- W3215487907 cites W2152638841 @default.
- W3215487907 cites W2153260254 @default.
- W3215487907 cites W2158507090 @default.
- W3215487907 cites W2160966131 @default.
- W3215487907 cites W2168207996 @default.
- W3215487907 cites W2287642689 @default.
- W3215487907 cites W2520740623 @default.
- W3215487907 cites W2715573044 @default.
- W3215487907 cites W2735736760 @default.
- W3215487907 cites W2782946598 @default.
- W3215487907 cites W2807767664 @default.
- W3215487907 cites W2890204506 @default.
- W3215487907 cites W2902664107 @default.
- W3215487907 cites W2912827267 @default.
- W3215487907 cites W2964335295 @default.
- W3215487907 cites W2980236528 @default.
- W3215487907 cites W2990334352 @default.
- W3215487907 cites W3036415057 @default.
- W3215487907 cites W3046800483 @default.
- W3215487907 cites W3098240284 @default.
- W3215487907 cites W3099100045 @default.
- W3215487907 cites W3099287625 @default.
- W3215487907 cites W3099836558 @default.
- W3215487907 cites W3100054267 @default.
- W3215487907 cites W3100086394 @default.
- W3215487907 cites W3100512461 @default.
- W3215487907 cites W3100847552 @default.
- W3215487907 cites W3100858899 @default.
- W3215487907 cites W3101490031 @default.
- W3215487907 cites W3101893366 @default.
- W3215487907 cites W3102281906 @default.
- W3215487907 cites W3102504011 @default.
- W3215487907 cites W3103740973 @default.
- W3215487907 cites W3103970226 @default.
- W3215487907 cites W3104054853 @default.
- W3215487907 cites W3104256320 @default.
- W3215487907 cites W3104549047 @default.
- W3215487907 cites W3104621534 @default.
- W3215487907 cites W3104662021 @default.
- W3215487907 cites W3104948779 @default.
- W3215487907 cites W3105094438 @default.
- W3215487907 cites W3106137340 @default.
- W3215487907 cites W3109791240 @default.
- W3215487907 cites W3111332701 @default.
- W3215487907 cites W3120594766 @default.
- W3215487907 cites W3124558775 @default.
- W3215487907 cites W3125203269 @default.
- W3215487907 cites W3125508207 @default.
- W3215487907 cites W3127053563 @default.
- W3215487907 cites W3131280568 @default.
- W3215487907 cites W3153383773 @default.