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researcher

J. Robrade

6 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author4
  • middle author2

Across the 6 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph4
  • astro-ph.SR2
ORCID 0000-0002-4939-8940
same name
  • J. Robrade — 1 paper, h 23

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20072009
most citedX-rays from RU Lupi - Accretion and winds in CTTS

82 citations · 228 across the 6 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2008★ 51 cited

Further X-ray detections of Herbig stars

B. Stelzer, J. Robrade, J. H. M. M. Schmitt +1

The interpretation of X-ray detections from Herbig Ae/Be stars is disputed as it is not clear if these intermediate-mass pre-main sequence stars are able to drive a dynamo and ensu…

astro-ph2008★ 11 cited

Quiescent X-ray emission from the M9 dwarf LHS 2065

J. Robrade, J. H. M. M. Schmitt

We investigate an archival XMM-Newton observation of LHS 2065, an ultracool dwarf with spectral type M9. We clearly detect LHS 2065 at soft X-ray energies in less than 1 h effectiv…

astro-ph2007★ 22 cited

Doppler imaging an X-ray flare on the ultrafast rotator BO Mic - A contemporaneous multiwavelength study using XMM-Newton and VLT

U. Wolter, J. Robrade, J. H. M. M. Schmitt +1

We present an analysis of contemporaneous photospheric, chromospheric and coronal structures on the highly active K-dwarf star BO Mic (Speedy Mic). We localize a moderate flare in…

astro-ph2007★ 82 cited

X-rays from RU Lupi - Accretion and winds in CTTS

J. Robrade, J. H. M. M. Schmitt

Using three XMM-Newton observations we study the X-ray emission of RU Lup, a accreting and wind-driving CTTS. In comparison with other bright CTTS we study possible signatures of a…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.