STAR FORMATION ACTIVITY OF CORES WITHIN INFRARED DARK CLOUDS

By E. Chambers, J. Jackson, J. Rathborne, R. Simon. 2009

192 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/ca2219ef50e47b58f47de30ca4f9943aa92f0994

How researchers see this paper

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

In Astronomy and Astrophysics

1. J. Jackson
2. G. Fuller
3. Nicolas Peretto
4. T. Pillai
5. J. Rathborne
6. R. Simon
7. L. Testi
8. L. Anderson

In Atmospheric Science

1. J. Jackson
2. B. Whitney
3. T. Pillai
4. G. Rieke
5. J. Bernard
6. Christoph Federrath

Citations in the corpus

• TADPOL: A 1.3 mm SURVEY OF DUST POLARIZATION IN STAR-FORMING CORES AND REGIONS (2013, background): “Water maser emission, massive CO outflows, and excess 4.5µm emission indicative of shocks have all been reported toward both MM1 and MM3 (Wang et al. 2006; Shepherd et al. 2007; Chambers et al. 2009; Sanhueza et al. 2010).”
• STAR FORMATION IN THE CENTRAL 400 PC OF THE MILKY WAY: EVIDENCE FOR A POPULATION OF MASSIVE YOUNG STELLAR OBJECTS (2009, methodology): “In particular, the correlation of 24µm point sources distributed toward infrared dark clouds with 4.5µm excess sources, thought to trace shock excited molecular emission, can be used to identify the earliest phase of massive star formation (Chambers et al. 2009).”
• CHEMISTRY IN INFRARED DARK CLOUD CLUMPS: A MOLECULAR LINE SURVEY AT 3 mm (2011, methodology): “We have carried out a multi-line survey at 3 mm toward 37 IRDCs, containing 159 clumps, in order to investigate the behavior of the different molecular tracers and search for chemical variations through an evolutionary sequence based on Spitzer IRAC and MIPS emission.”
• THE GREEN BANK TELESCOPE H ii REGION DISCOVERY SURVEY. II. THE SOURCE CATALOG (2011, background): “IRDCs are associated with the earliest phases of star formation (Chambers et al. 2009; Rathborne et al. 2010).”
• THE “NESSIE” NEBULA: CLUSTER FORMATION IN A FILAMENTARY INFRARED DARK CLOUD (2009, background): “Specifically, many cores show the presence of excess 4.5 µm emission called “green fuzzies,” which indicates shocked gas (e.g., Noriega-Crespo et al. 2004; Marston et al. 2004), and bright 24 µm point sources, which indicate an embedded protostar (e.g., Chambers et al. 2009).”
• Characterizing precursors to stellar clusters with Herschel (2011, methodology): “We create star formation tracer label maps for the MIPS 24 µm emission, 8 µm emission, EGOs (Cyganowski et al. 2008; Chambers et al. 2009), and 6.7 GHz methanol maser emission (Pestalozzi et al. 2005).”
• A CLASS I AND CLASS II CH3OH MASER SURVEY OF EGOs FROM THE GLIMPSE SURVEY (2009, background): “Such features are known as " Extended Green Objects (EGOs) " (Cyganowski et al. 2008) or " green fuzzies " (Chambers et al. 2009), for the common coding of the [4.5] band as green in three-color IRAC images.”