Physical processes in star formation
P Girichidis, SSR Offner, AG Kritsuk, RS Klessen… - Space Science …, 2020 - Springer
Star formation is a complex multi-scale phenomenon that is of significant importance for
astrophysics in general. Stars and star formation are key pillars in observational astronomy …
astrophysics in general. Stars and star formation are key pillars in observational astronomy …
The search for infrared protostars
CG Wynn-Williams - In: Annual review of astronomy and …, 1982 - adsabs.harvard.edu
A review of the search for infrared sources in star-forming regions, and studies of these
sources and nearby interstellar matter, are presented. Particular attention is given to those …
sources and nearby interstellar matter, are presented. Particular attention is given to those …
The observed spiral structure of the Milky Way
LG Hou, JL Han - Astronomy & Astrophysics, 2014 - aanda.org
Context. The spiral structure of the Milky Way is not yet well determined. The keys to
understanding this structure are to increase the number of reliable spiral tracers and to …
understanding this structure are to increase the number of reliable spiral tracers and to …
A magnetized jet from a massive protostar
C Carrasco-González, LF Rodríguez, G Anglada… - Science, 2010 - science.org
Synchrotron emission is commonly found in relativistic jets from active galactic nuclei
(AGNs) and microquasars, but so far its presence in jets from young stellar objects (YSOs) …
(AGNs) and microquasars, but so far its presence in jets from young stellar objects (YSOs) …
The initial configuration of young stellar clusters: A K-band number counts analysis of the surface density of stars
RA Gutermuth, ST Megeath, JL Pipher… - The Astrophysical …, 2005 - iopscience.iop.org
We present an analysis of stellar distributions for the young stellar clusters GGD 12-15, IRAS
20050+ 2720, and NGC 7129, which range in far-IR luminosity from 227 to 5.68× 10 3 L☉ …
20050+ 2720, and NGC 7129, which range in far-IR luminosity from 227 to 5.68× 10 3 L☉ …
VLBA determination of the distance to nearby star-forming regions. IV. A preliminary distance to the proto-Herbig AeBe Star EC 95 in the Serpens core
S Dzib, L Loinard, AJ Mioduszewski… - The Astrophysical …, 2010 - iopscience.iop.org
ABSTRACT Using the Very Long Base Array, we observed the young stellar object EC 95 in
the Serpens cloud core at eight epochs from 2007 December to 2009 December. Two …
the Serpens cloud core at eight epochs from 2007 December to 2009 December. Two …
Mass spectra of young stars
RB Larson - Monthly Notices of the Royal Astronomical Society, 1982 - academic.oup.com
In an effort to understand the factors that determine the initial mass function of stars, the
available data on the mass spectra of young stars in different regions have been studied for …
available data on the mass spectra of young stars in different regions have been studied for …
The Arcetri atlas of H2O maser sources
G Comoretto, F Palagi, R Cesaroni… - … Series (ISSN 0365 …, 1990 - adsabs.harvard.edu
Results are reported from a 22.2-GHz H2O line survey of all the known maser sources north
of-30 deg. Of the 509 sources observed, 203 were detected with an average detection limit …
of-30 deg. Of the 509 sources observed, 203 were detected with an average detection limit …
(C-13) O and (C-12) O observations of cold IRAS unidentified point sources in the Galaxy
F Casoli, C Dupraz, M Gerin, F Combes… - … vol. 169, no. 1-2, Nov …, 1986 - adsabs.harvard.edu
Observations of 13 CO and 12 CO have been made in the direction of 96 infrared sources
selected from the IRAS point-source catalogue, and having a flux density at 100 μm greater …
selected from the IRAS point-source catalogue, and having a flux density at 100 μm greater …
Resolving the Polarized Dust Emission of the Disk around the Massive Star Powering the HH 80–81 Radio Jet
Here we present deep (16 μJy beam− 1), very high (40 mas) angular resolution 1.14 mm,
polarimetric, Atacama Large Millimeter/submillimeter Array (ALMA) observations toward the …
polarimetric, Atacama Large Millimeter/submillimeter Array (ALMA) observations toward the …