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Peter S. Conti

1 paper here

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  • last author1

Across the 1 of 1 paper where every author was matched, so the position is known.

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  • astro-ph1

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most citedOn the role of the WNH phase in the evolution of very massive stars: Enabling the LBV instability with feedback

105 citations · 105 across the 1 of their papers we have counts for

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3 papers · 1 filter

astro-ph2008★ 28 cited

High Spatial Resolution Spectroscopy of W51 IRS2E and IRS2W: Two Very Massive Young Stars in Early Formation Stages

C. L. Barbosa, R. D. Blum, P. S. Conti +2

We present K-band spectra of the near infrared counterparts to IRS2E and IRS2W which is associated with the ultracompact HII region W51d, both of them embedded sources in the Gal…

astro-ph2008

The Stellar Content of Obscured Galactic Giant HII Regions. VI: W51A

E. Figueredo, R. D. Blum, A. Damineli +2

We present K-band spectra of newly born OB stars in the obscured Galactic giant H II region W51A and ~ 0.8'' angular resolution images in the J, H and K_S-bands. Four objects have…

astro-ph2008★ 105 cited

On the role of the WNH phase in the evolution of very massive stars: Enabling the LBV instability with feedback

Nathan Smith, Peter S. Conti

(abridged) We propose the new designation ``WNH'' for luminous Wolf-Rayet (WR) stars of the nitrogen sequence with H in their spectra. These are commonly called WNL stars (e.g., WN…

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