scholarly journals The WISE Census of Young Stellar Objects in Canis Major

2015 ◽  
Vol 10 (S314) ◽  
pp. 63-64
Author(s):  
W. J. Fischer ◽  
D. L. Padgett ◽  
K. R. Stapelfeldt
Keyword(s):  
Molecular Clouds ◽  
Young Stellar Objects ◽  
Wide Field ◽  
Spitzer Space Telescope ◽  
Stellar Objects ◽  
Space Telescope ◽  
Infrared Survey

AbstractWhile searches for young stellar objects (YSOs) with the Spitzer Space Telescope focused on known molecular clouds, photometry from the Wide-field Infrared Survey Explorer (WISE) can be used to extend the search to the entire sky. As a precursor to more expansive searches, we present results for a 100 deg2 region centered on the Canis Major clouds.

scholarly journals The WISE Census of Young Stellar Objects and Clusters in Canis Major

2015 ◽  
Vol 11 (S315) ◽  
Author(s):  
W. J. Fischer ◽  
D. L. Padgett ◽  
K. R. Stapelfeldt
Keyword(s):  
Molecular Clouds ◽  
Photometric Data ◽  
Young Stellar Objects ◽  
Wide Field ◽  
Stellar Objects ◽  
Infrared Survey

AbstractThe photometric data returned by WISE, the Wide-field Infrared Survey Explorer, can be used to search the sky for young stellar objects (YSOs) away from the molecular clouds studied in detail by Spitzer and Herschel. We present updated results for a 100 deg2 region centered on Canis Major, including a look at the clustering properties of YSOs in the region.

scholarly journals Degenerates with Dusty Disks: White Dwarfs and Cataclysmic Variables in the Infrared

2012 ◽  
Vol 8 (S290) ◽  
pp. 121-124
Author(s):  
D. W. Hoard
Keyword(s):  
White Dwarfs ◽  
Cataclysmic Variables ◽  
Wide Field ◽  
Spitzer Space Telescope ◽  
Space Telescope ◽  
Infrared Observations ◽  
Compact Binaries ◽  
Dusty Disks ◽  
Infrared Survey

AbstractRecent infrared observations, particularly from the Spitzer Space Telescope and Wide-field Infrared Survey Explorer, of white dwarfs, cataclysmic variables and other interacting compact binaries, have revealed the presence of dust in many systems. I briefly review the discovery and observational properties of dust around white dwarfs and cataclysmic variables.

scholarly journals SK 1: A possible case of triggered star formation in perseus

2006 ◽  
Vol 2 (S237) ◽  
pp. 217-221
Author(s):  
Miriam Rengel ◽  
Klaus Hodapp ◽  
Jochen Eislöffel
Keyword(s):  
Star Formation ◽  
Molecular Clouds ◽  
Thermal Emission ◽  
Young Stellar Objects ◽  
Wide Field ◽  
Dust Shell ◽  
Stellar Objects ◽  
Star Forming ◽  
Star Forming Regions ◽  
Suitable Target

AbstractAccording to a triggered star formation scenario (e.g. Martin-Pintado & Cernicharo 1987) outflows powered by young stellar objects shape the molecular clouds, can dig cavities, and trigger new star formation. NGC 1333 is an active site of low- and intermediate star formation in Perseus and is a suggested site of self-regulated star formation (Norman & Silk 1980). Therefore it is a suitable target for a study of triggered star formation (e.g. Sandell & Knee 2001, SK1). On the other hand, continuum sub-mm observations of star forming regions can detect dust thermal emission of embedded sources (which drive outflows), and further detailed structures.Within the framework of our wide-field mapping of star formation regions in the Perseus and Orion molecular clouds using SCUBA at 850 and 450 μm, we mapped NCG 1333 with an area of around 14′× 21′. The maps show more structure than the previous maps of the region observed in sub-mm. We have unveiled the known embedded SK 1 source (in the dust shell of the SSV 13 ridge) and detailed structure of the region, among some other young protostars.In agreement with the SK 1 observations, our map of the region shows lumpy filaments and shells/cavities that seem to be created by outflows. The measured mass of SK 1 (~0.07 M) is much less than its virial mass (~0.2-1 M). Our observations support the idea of SK 1 as an event triggered by outflow-driven shells in NGC 1333 (induced by an increase in gas pressure and density due to radiation pressure from the stellar winds that have presumably created the dust shell). This kind of evidences provides a more thorough understanding of the star formation regulation processes.

scholarly journals Triggered star formation in a cometary atomic/molecular cloud in the Cep OB3 association

2019 ◽  
Vol 489 (4) ◽  
pp. 4809-4816 ◽  
Author(s):  
Brandon Marshall ◽  
C R Kerton
Keyword(s):  
Star Formation ◽  
Galactic Plane ◽  
Initial Conditions ◽  
Young Stellar Objects ◽  
Wide Field ◽  
Infrared Source ◽  
Stellar Objects ◽  
Iras Source ◽  
Infrared Observations ◽  
Infrared Survey

ABSTRACT We present a study of a small atomic/molecular cometary cloud associated with the infrared source IRAS 23153+6938. The cloud is located 70 pc from the massive O-type stars in the Cepheus OB3 association, and is very likely an excellent example of triggered star formation via radiation-driven implosion (RDI). The cloud was studied using $\rm{H\,\small{I}}$ and 12CO data from the Canadian Galactic Plane Survey (CGPS) and infrared observations from the Wide-field Infrared Survey Explorer (WISE) telescope. The molecular mass is approximately MH2 = 350 ± 45 M$\odot$, and we find that the single IRAS source is actually the centre of a small cluster of class I and class II young stellar objects (YSOs). To compare with theory, we make reasonable estimates for the cometary cloud’s initial conditions and find that the cloud is located within the correct theoretical phase space for RDI to occur. In addition, both the morphology of the cloud and the location of different YSO classes relative to the cloud match what would be expected for RDI. We conclude that RDI is the most likely explanation for star formation within the cloud, and we suggest that similar studies of molecular clouds associated with nearby OB associations may be able to identify comparable examples.

scholarly journals WIDE-FIELD INFRARED SURVEY EXPLORER OBSERVATIONS OF YOUNG STELLAR OBJECTS IN THE WESTERN CIRCINUS MOLECULAR CLOUD

2011 ◽  
Vol 733 (1) ◽  
pp. L2 ◽  
Author(s):  
Wilson M. Liu ◽  
Deborah L. Padgett ◽  
David Leisawitz ◽  
Sergio Fajardo-Acosta ◽  
Xavier P. Koenig
Keyword(s):  
Molecular Cloud ◽  
Young Stellar Objects ◽  
Wide Field ◽  
Stellar Objects ◽  
Infrared Survey

scholarly journals WIDE-FIELD INFRARED SURVEY EXPLOREROBSERVATIONS OF YOUNG STELLAR OBJECTS IN THE LYNDS 1509 DARK CLOUD IN AURIGA

2014 ◽  
Vol 147 (6) ◽  
pp. 133 ◽  
Author(s):  
Wilson M. Liu ◽  
Deborah L. Padgett ◽  
Susan Terebey ◽  
John Angione ◽  
Luisa M. Rebull ◽  
...  
Keyword(s):  
Young Stellar Objects ◽  
Wide Field ◽  
Dark Cloud ◽  
Stellar Objects ◽  
Infrared Survey

scholarly journals The Galactic star formation rate as seen by the Spitzer Space Telescope

2009 ◽  
Vol 5 (H15) ◽  
pp. 799-799
Author(s):  
Thomas P. Robitaille ◽  
Barbara A. Whitney
Keyword(s):  
Star Formation ◽  
Star Formation Rate ◽  
Formation Rate ◽  
Young Stellar Objects ◽  
Spitzer Space Telescope ◽  
Stellar Objects ◽  
Space Telescope ◽  
Preliminary Results ◽  
A Value ◽  
The Galaxy

AbstractWe present preliminary results of a study to determine the star formation rate of the Galaxy using a census of young stellar objects (YSOs) in the Spitzer/GLIMPSE and MIPSGAL surveys, which cover nearly 300 square degrees of the Galactic mid-plane. We find a value of 1.7 M⊙/yr, consistent with independent estimates.

scholarly journals The relationship between mid-infrared and sub-millimetre variability of deeply embedded protostars

2020 ◽  
Vol 495 (4) ◽  
pp. 3614-3635 ◽  
Author(s):  
Carlos Contreras Peña ◽  
Doug Johnstone ◽  
Giseon Baek ◽  
Gregory J Herczeg ◽  
Steve Mairs ◽  
...  
Keyword(s):  
Young Stellar Objects ◽  
Time Variability ◽  
Wide Field ◽  
Stellar Objects ◽  
Mid Infrared ◽  
James Clerk Maxwell ◽  
Secular Variability ◽  
The Relationship ◽  
Exact Scaling ◽  
Infrared Survey

ABSTRACT We study the relationship between the mid-infrared (mid-IR) and sub-millimetre (sub-mm) variability of deeply embedded protostars using the multi-epoch data from the Wide-field Infrared Survey Explorer (WISE/NEOWISE) and the ongoing James Clerk Maxwell Telescope (JCMT) Transient Survey. Our search for signs of stochastic (random) and/or secular (roughly monotonic in time) variability in a sample of 59 young stellar objects (YSOs) revealed that 35 are variable in at least one of the two surveys. This variability is dominated by secular changes. Of those objects with secular variability, 14 objects ($22{{\ \rm per\ cent}}$ of the sample) show correlated secular variability over mid-IR and sub-mm wavelengths. Variable accretion is the likely mechanism responsible for this type of variability. Fluxes of YSOs that vary in both wavelengths follow a relation of log10F4.6(t) = ηlog10F850(t) between the mid-IR and sub-mm, with η = 5.53 ± 0.29. This relationship arises from the fact that sub-mm fluxes respond to the dust temperature in the larger envelope whereas the mid-IR emissivity is more directly proportional to the accretion luminosity. The exact scaling relation, however, depends on the structure of the envelope, the importance of viscous heating in the disc, and dust opacity laws.

scholarly journals A Spitzer Space Telescope survey of massive young stellar objects in the G333.2−0.4 giant molecular cloud

2011 ◽  
Vol 419 (1) ◽  
pp. 211-237 ◽  
Author(s):  
Janet P. Simpson ◽  
Angela S. Cotera ◽  
Michael G. Burton ◽  
Maria R. Cunningham ◽  
Nadia Lo ◽  
...  
Keyword(s):  
Molecular Cloud ◽  
Young Stellar Objects ◽  
Spitzer Space Telescope ◽  
Stellar Objects ◽  
Space Telescope ◽  
Giant Molecular Cloud

scholarly journals Hα emission-line stars in molecular clouds

2019 ◽  
Vol 630 ◽  
pp. A90 ◽  
Author(s):  
Bertil Pettersson ◽  
Bo Reipurth
Keyword(s):  
Molecular Clouds ◽  
Young Stellar Objects ◽  
Be Stars ◽  
Stellar Objects ◽  
Strong Concentration ◽  
Ob Stars ◽  
Star Forming ◽  
Hα Emission ◽  
Objective Prism ◽  
Emission Stars

A deep objective-prism survey for Hα emission stars towards the Canis Major star-forming clouds was performed. A total of 398 Hα emitters were detected, 353 of which are new detections. There is a strong concentration of these Hα emitters towards the molecular clouds surrounding the CMa OB1 association, and it is likely that these stars are young stellar objects recently born in the clouds. An additional population of Hα emitters is scattered all across the region, and probably includes unrelated foreground dMe stars and background Be stars. About 90% of the Hα emitters are detected by WISE, of which 75% was detected with usable photometry. When plotted in a WISE colour–colour diagram it appears that the majority are Class II YSOs. Coordinates and finding charts are provided for all the new stars, and coordinates for all the detections. We searched the Gaia-DR2 catalogue and from 334 Hα emission stars with useful parallaxes, we selected a subset of 98 stars that have parallax errors of less than 20% and nominal distances in the interval 1050 to 1350 pc that surrounds a strong peak at 1185 pc in the distance distribution. Similarly, Gaia distances were obtained for 51 OB-stars located towards Canis Major and selected with the same parallax errors as the Hα stars. We find a median distance for the OB stars of 1182 pc, in excellent correspondence with the distance from the Hα stars. Two known runaway stars are confirmed as members of the association. Finally, two new Herbig-Haro objects are identified.

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