activity
20042010
most citedOn the internal structure of starless cores. II. A molecular survey of L1498 and L1517B

204 citations · 500 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2010★ 33 cited

Variations in H2O+/H2O ratios toward massive star-forming regions

F. Wyrowski, F. van der Tak, F. Herpin +63

Early results from the Herschel Space Observatory revealed the water cation H2O+ to be an abundant ingredient of the interstellar medium. Here we present new observations of the H2…

astro-ph.GA2010★ 107 cited

Water cooling of shocks in protostellar outflows: Herschel-PACS map of L1157

B. Nisini, M. Benedettini, C. Codella +62

In the framework of the Water in Star-forming regions with Herschel (WISH) key program, maps in water lines of several outflows from young stars are being obtained, to study the wa…

astro-ph.GA2010★ 37 cited

Water abundance variations around high-mass protostars: Herschel-HIFI observations of the DR21 region

F. F. S. van der Tak, M. G. Marseille, F. Herpin +1

Water is a key molecule in the star formation process, but its spatial distribution in star-forming regions is not well known. We study the distribution of dust continuum and H2O a…

astro-ph2006★ 204 cited

On the internal structure of starless cores. II. A molecular survey of L1498 and L1517B

M. Tafalla, J. Santiago, P. C. Myers +3

[Abridged] We present a molecular survey of the starless cores L1498 and L1517B. These cores have been selected for their relative isolation and close-to-round shape, and they have…

astro-ph2004★ 46 cited

A highly collimated, extremely high velocity outflow in Taurus

M. Tafalla, J. Santiago, D. Johnstone +1

We present the first case of a highly collimated, extremely high velocity bipolar outflow in Taurus. It is powered by the low-luminosity (0.4 L_sun) source IRAS 04166+2706 and cont…

astro-ph2004★ 73 cited

L1521E: the first starless core with no molecular depletion

M. Tafalla, J. Santiago

L1521E seems unique among starless cores. It stands out in a distribution of a ratio (R) that we define to asses core evolution, and which compares the emission of the easily-deple…