IRAS07027$-$7934: the link between OH/IR stars and carbon-rich planetary nebulae Albert A. Zijlstra$^1$, Mike J. Gaylard$^2$, Peter te Lintel Hekkert$^3$, John Menzies$^1$, L.-\AA.\ Nyman$^4$, Hugo E. Schwarz$^4$ IRAS07027-7934, a young planetary nebula with a [WC11] central star, is found to show a strong $1612 \mhz$ OH maser, as well as weak CO emission. PAH features indicate that the ionized region is carbon-rich. ...
... astro-ph . ... SAI VO . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . Normalized to: Gaylard, M. 15 article(s) in total . 328 co-authors, from 1 to 10 common article(s). ... Bergano, Miguel. ... Brun, F.. ... Cerruti, Miguel Angel. ... Jung, I.. Jung, Taehyun. ... Martin, Jerome. ... Reimer, Olaf. ... van Ardenne, A.. - . van der Horst, A. J.. - . van der Walt, D. J.. - . van Eldik, C.. - . ... van Leeuwen, Joeri. ...
Astronomy & Astrophysics manuscript no. rcw79f2 (DOI: will be inserted by hand later) September 12, 2005 Triggered massive-star formation on the borders of Galactic H II regions II. ... All these facts strongly indicate that the massive-star formation observed at the border of the H II region RCW 79 has been triggered by its expansion, most probably by the collect and collapse process. ... Stars: formation Stars: early-type ISM: H II regions ISM: individual: RCW 79 1. ... Fig. ... This in- Fig. ...
... Here we present and discuss Vela Jr. properties revealed by these multiwavelength observations, and confront them with the SNR model expectations. ... Multiple observations of Vela Jr. in the radio band confirmed the shell-like structure and supported the identification of RX J0852.0-4622 as a SNR [8,11,12,13,14,16,46]. ... The X-ray emission line feature at 4.2 keV found by ASCA [48] in the NW rim spectrum of RX J0852.0-4622 was confirmed by XMM-Newton data (Fig. 4, 5, and [22]), and by Chandra [4]...
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