About: The X-ray emission from Z Canis Majoris during an FUor-like outburst and the detection of its X-ray jet     Goto   Sponge   NotDistinct   Permalink

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  • We observed the FUor object Z CMa during optical outburst and quiescence with Chandra. No significant changes in X-ray brightness and spectral shape were found, suggesting that the X-ray emission is coronal. The binary nature of Z CMa makes the origin of the X-ray source ambiguous. However, the moderate hydrogen column density derived from our data makes it unlikely that the embedded primary star is the X-ray source. The secondary star, which is the FUor object, is thus responsible for both the X-ray emission and the ongoing accretion outburst, which seem, however, to be unrelated phenomena. The secondary is also known to drive a large outflow and jet, which we detect here for the first time in X-rays. The distance of the X-ray emitting outflow source to the central star is greater than in jets of low-mass stars.
  • We observed the FUor object Z CMa during optical outburst and quiescence with Chandra. No significant changes in X-ray brightness and spectral shape were found, suggesting that the X-ray emission is coronal. The binary nature of Z CMa makes the origin of the X-ray source ambiguous. However, the moderate hydrogen column density derived from our data makes it unlikely that the embedded primary star is the X-ray source. The secondary star, which is the FUor object, is thus responsible for both the X-ray emission and the ongoing accretion outburst, which seem, however, to be unrelated phenomena. The secondary is also known to drive a large outflow and jet, which we detect here for the first time in X-rays. The distance of the X-ray emitting outflow source to the central star is greater than in jets of low-mass stars. (en)
Title
  • The X-ray emission from Z Canis Majoris during an FUor-like outburst and the detection of its X-ray jet
  • The X-ray emission from Z Canis Majoris during an FUor-like outburst and the detection of its X-ray jet (en)
skos:prefLabel
  • The X-ray emission from Z Canis Majoris during an FUor-like outburst and the detection of its X-ray jet
  • The X-ray emission from Z Canis Majoris during an FUor-like outburst and the detection of its X-ray jet (en)
skos:notation
  • RIV/00216224:14310/09:00035658!RIV10-MSM-14310___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • S
http://linked.open...iv/cisloPeriodika
  • 499
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 352144
http://linked.open...ai/riv/idVysledku
  • RIV/00216224:14310/09:00035658
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • X-rays: stars; accretion; accretion disks; stars: pre-main sequence; stars: variables: general; stars: activity; stars: winds; outflows (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [EFBF931B9DF9]
http://linked.open...i/riv/nazevZdroje
  • Astronomy and Astrophysics
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 2009
http://linked.open...iv/tvurceVysledku
  • Hubrig, Swetlana
  • Mikulášek, Zdeněk
  • Stelzer, Beate
  • Micela, G.
  • Schöller, M.
  • Orlando, S.
http://linked.open...ain/vavai/riv/wos
  • 000266730500017
issn
  • 0004-6361
number of pages
http://localhost/t...ganizacniJednotka
  • 14310
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