activity
20022008
most citedThe Cassiopeia A Supernova was of Type IIB

324 citations · 708 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph2008213 cited

Tycho Brahe's 1572 supernova as a standard type Ia explosion revealed from its light echo spectrum

Oliver Krause, Masaomi Tanaka, Tomonori Usuda +4

Type Ia supernovae (SNe Ia) are thermonuclear explosions of white dwarf stars in close binary systems. They play an important role as cosmological distance indicators and have led…

astro-ph200895 cited

Absorption Line Survey of H3+ toward the Galactic Center Sources II. Eight Infrared Sources within 30 pc of the Galactic Center

Miwa Goto, T. Usuda, T. Nagata +7

Infrared absorption lines of H3+, including the metastable R(3,3)l line, have been observed toward eight bright infrared sources associated with hot and massive stars located in an…

astro-ph2008324 cited

The Cassiopeia A Supernova was of Type IIB

Oliver Krause, Stephan M. Birkmann, Tomonori Usuda +4

Cassiopeia A is one of the youngest supernova remnants known in the Milky Way and a unique laboratory for supernova physics. We present an optical spectrum of the Cassiopeia A supe…

astro-ph200718 cited

A Search for NIR Molecular Hydrogen Emission in the CTTS LkHa 264 and the debris disk 49 Cet

A. Carmona, M. E van den Ancker, Th. Henning +3

We report on the first results of a search for H2 emission from protoplanetary disks using CRIRES, ESO's new VLT high resolution NIR spectrograph. We observed the CTTS LkHa 264 and…

astro-ph200758 cited

A Search for Mid-Infrared Molecular Hydrogen Emission from Protoplanetary Disks

A. Carmona, M. E van den Ancker, Th. Henning +6

We observed the Herbig Ae/Be stars UX Ori, HD 34282, HD 100453, HD 101412, HD 104237 and HD 142666, and the T Tauri star HD 319139 and searched for H2 0-0 S(2) emission at 12.278 m…

astro-ph2005

Search for H3+ in HD141569A

M. Goto, T. R. Geballe, B. J. McCall +5

A search for H3+ line emission, reported to have been detected toward the young star HD 141569A and possibly originating in a clump of planet-forming gas orbiting the star, has yie…