Handbook of Star Forming Regions, Volume I: The Northern Sky

By B. Reipurth. 2008

311 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/2427e3637081e271e2cffd1549ffbd9fb6a4e624

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Citations in the corpus

The relation between the most-massive star and its parental star cluster mass (2009, background): “2001; Weidner et al. 2007). The exception are four objects which this sample has in common with the near infra-red study of young star-forming regions by Wang & Looney (2007) and which are all included in our study. Based on similar arguments Maschberger & Clarke (2008) also excluded the Testi et al”
A compendium of distances to molecular clouds in the Star Formation Handbook (2020, methodology): “The Star Formation Handbook, divided into two volumes for the Northern (Reipurth 2008a) and Southern (Reipurth 2008b) sky, contains around sixty of the most important star forming regions within 2 kpc. Written by a team of 105 authors, the Handbook spans 1900 pages, and includes the most…”
THE TUCANA/HOROLOGIUM, COLUMBA, AB DORADUS, AND ARGUS ASSOCIATIONS: NEW MEMBERS AND DUSTY DEBRIS DISKS (2011, methodology): “Excepting the Sun, it is difficult to deduce even a moderately accurate age of an individual star. Astronomers have circumvented this problem by studying stars in rich open and globular clusters. Excepting the Hyades, no such clusters exist within 100 pc of Earth. Fortunately, beginning in the late ”
An ALMA study of the Orion Integral Filament: I. Evidence for narrow fibers in a massive cloud (2018, background): “(2016); (6)Bally et al. (1987); (7)Johnstone & Bally (1999); (8)Palmeirim et al.”
ESTIMATING THE STAR FORMATION RATE AT 1 kpc SCALES IN NEARBY GALAXIES (2012, background): “…between 24µm emission and sites of active star formation (e.g., Calzetti et al. 2005; Alonso-Herrero et al. 2006; Pérez-González et al. 2006; Prescott et al. 2007) and it has been used extensively to investigate the correlations between gas and star formation (e.g., Kennicutt et al.…”
Probing the evolution of molecular cloud structure: From quiescence to birth (2009, background): “…(9) Obayashi et al. (1998) (10) Corradi et al. (1997) (11) Burrows et al. (1993) (12) Cernis (1993) (13) Crawford et al. (1970) (14) Lada et al. (2009). b An order-of-magnitude estimate of the pre-main-sequence star population in the clouds, based on Reipurth (2008). c No good fit was achieved.”