activity
19952026
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 38.1k across the 501 of their papers we have counts for

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Showing 2004 · astro-phShow all

6 papers · 2 filters

astro-ph2004★ 86 cited

Search for massive protostellar candidates in the southern hemisphere: I. Association with dense gas

F. Fontani, M. T. Beltran, J. Brand +4

(Abridged) We have observed CS and C17O lines, and 1.2 mm cont. emission towards a sample of 130 high-mass protostellar candidates with DEC<-30 deg. This is the first step of the s…

astro-ph2004★ 41 cited

Diamonds in HD 97048

E. Habart, L. Testi, A. Natta +1

We present adaptive optics high angular resolution ($\sim0\farcs$1) spectroscopic observations in the 3 m region of the Herbig Ae/Be star HD 97048. For the first time, we spatia…

astro-ph2004★ 410 cited

Accretion in Brown Dwarfs: an Infrared View

A. Natta, L. Testi, J. Muzerolle +3

This paper presents a study of the accretion properties of 19 very low mass objects (Mstar .01-0.1 Msun) in the regions Chamaeleon I and rho-Oph For 8 objects we obtained high reso…

astro-ph2004★ 23 cited

Nature of two massive protostellar candidates: IRAs 21307+5049 and IRAS 22172+5549

F. Fontani, R. Cesaroni, L. Testi +4

We present observations of continuum and molecular lines towards the protostar candidates IRAS 21307+5049 and IRAS 22172+5549. Single-dish maps in the 12CO(2--1), C18O(2--1), HCO+(…

astro-ph2004★ 101 cited

The Origin of Massive O-type Field Stars. Part I: A Search for Clusters

W. J. de Wit, L. Testi, F. Palla +2

We present a study aimed at clarifying the birthplace for 43 massive O-type field stars. In this first paper we present the observational part: a search for stellar clusters near t…

astro-ph2004★ 11 cited

Detection of Knots and Jets in IRAS 06061+2151

B. G. Anandarao, A. Chakraborty, D. K. Ojha +1

We report detection of a Young Stellar Object with an evidence for an outflow in the form of knots in the molecular hydrogen emission line (2.121 micron) towards the massive star f…