Difference between revisions of "Jackie BRC 38"
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== Articles == | == Articles == | ||
| + | {| {{table}} | ||
| + | | align="center" style="background:#f0f0f0;"|'''http://arxiv.org/pdf/1201.2704.pdf''' | ||
| + | | align="center" style="background:#f0f0f0;"|'''saurin 2012''' | ||
| + | | align="center" style="background:#f0f0f0;"|'''the embedded cluster or assoiciation trumpter 37 in ir 1396''' | ||
| + | | align="center" style="background:#f0f0f0;"|'''2MASS obsevations of BRC 38''' | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/1103.1646v1.pdf||Barensten et al. 2011||T tauri candidates and accretion rates using IPHAS: method and application to IC 1396||Includes BRC 38 which is called cloud E; Looking for YSOs in all of 1396; list 158 candidates; uses IPHAS survey data - Halpha, r, I filters on isaac newton telescope | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/1005.1841v1.pdf||choudhury 2010||Triggered star formation and YSO population in Bright Rimmed SRO 38||44 YSOs identified in brc 38 - evidence for radiation driven implosion (RDI); spizter IRAC & MIPS data, optical BVRI | ||
| + | |- | ||
| + | | ||Morgan et al. 2010||Ammonia observations of bright-rimmed clouds: establishing a sample of triggered protostars||Radio observations (Green Bank) of brcs; furthering earlier work of morgan, confirming brc is triggered star formation site | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/1005.0947v1.pdf||Crimier 2010||Physical structure of the envelopes of intermediate-mass protostars||a study that says that the mass of the final star of a protostar is linked to the mass of the envelope around the protostar, not the density of the parent cloud - backbground on IM protostars?? | ||
| + | |- | ||
| + | | http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2010ASInC...1...19O&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Ogura 2010||Triggered star formation assoicated with HII regions||Not really about BRC 38 but discusses curent state of triggered star formation theory | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/0902.4543v1.pdf||beltran et al. 2009||The stellar population and complex structure of the bright-rimmed cloud ic 1396N||A study through J< H< K\' filters; 736 sources found in all 3 bands (filters); h2 emission shows jet like structure | ||
| + | |- | ||
| + | | http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2009MNRAS.400.1726M||Morgan 2009||CO observations towards bright-rimmed clouds||can\'t get paper | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/0909.2267v1.pdf||fuente 2009||Dissecting an intermediate-mass (IM) prostar||A look at IRAS 21391+5802 emissions of N2H+, CH3CN, CS, BIMA (1.2mm & 3.1mm) | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/0909.3312v1.pdf||Wang 2009||The relation between 13CO j=2-1 line width in moelcular clouds and bolometric luminosity of associated IRAS sources||IRAS 21391+5802 - suggests that it is a star forming cluster where high-mass stars will form | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/0903.2122v1.pdf||Chauhan 2009||Triggered star formation & evolution of t-tauri stars in and around BRC||Study that looked at ages of star forming clusters. Seems to be a lot of background materials on BRC 38 | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/0711.0775v1.pdf||Morgan 2007||A scuba survey of BRC||BRC 38 included in this study with SUBA data (submillimeter - microwave??); Classified as type B (tightly curved rims) which may be related to the strength of the ioisation field it is in | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/0705.2663v1.pdf||Neri 2007||The IC 1396N proto-cluster at a scale of ~250 AU||observations in millimeter range to help develop understanding of formation of clusters vs individual star formation | ||
| + | |- | ||
| + | | |||||| | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/astro-ph/0607006v2.pdf||Getman 2007||X-ray study of triggered star formation and protostars in IC 1396N||x-ray sources in the globule of ic 1396N; good pictures to help with the visualization of 1396N and these sources; evidence of sequential star formation | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/astro-ph/0702696v1.pdf||Patel 2007||Submillimeter array observations of 321 ghz water maser emission in cepheus a||No don\'t think there is anything here | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/astro-ph/0611634v1.pdf||Connelley 2006||Infrared Nebulae around Young stellar objects||IRAS 21391+5802 - images show jet-like nebula and large patches of nebulosity | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/astro-ph/0508446v1.pdf||valdettaro 2005||h2o maser emission from bright rimmed clouds in the northern hemisphere||H2O maser studied in brc 38; points to paper Valdettaro et al. 2005b | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/astro-ph/0407102v1.pdf||Beltran 2004||The dense moelcular cores in IRAS 21391 +5802 region||Three sources found with BIMA (??) observations in 21391+5802; Hard to read as they are trying to use data to fit/model how gas is emitted from the core | ||
| + | |- | ||
| + | | http://iopscience.iop.org/1538-4357/593/1/L47/pdf/17405.web.pdf||Reipurth 2003||Blowout from IC 1396N: The emergence of Herbig-Haro flows from a cloud core||Herbig-Haro flow (HH 777) found coming out of ic 1396N; located at 214041.6+581638 (in IR, I think) | ||
| + | |- | ||
| + | | http://adsabs.harvard.edu/full/2002aprm.conf..191O||Ogura, et el 2002||A large number of Halpha emission stars and Herbig-Haro objects in and around BRC||short (2 pages) listing observations of halpha emission stars - brc 38 has 7 | ||
| + | |- | ||
| + | | http://arxiv.org/pdf/astro-ph/0203206v1.pdf||Beltran et al. 2002||IRAS 21391+5802: The Molecular Outflow and its Exciting source||VLA and BIMA observations of dust and gas surrounding IRAS source; 3 sources isolated with BIMA, each a YSO | ||
| + | |- | ||
| + | | http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2001A%26A...376..271CFUL||Codella 2001||Star formation in the BRC of IC 1396N||The density of several different molecular outflows (dense areas of particular molecules)in the globule looked at with 30m IRAM and OVRO interferometer. Demonstrates this area very complex. | ||
| + | |- | ||
| + | | http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2001A%26A...376..553N&db_key=AST&nosetcookie=1||Nisini 2001||Multiple H2 protostellar jets in the bright-rimmed globule IC 1396-N||1st detection of H2 jets from YSO. Are these HH objects? | ||
| + | |- | ||
| + | | http://iopscience.iop.org/0004-637X/526/1/236/pdf/39770.web.pdf||Slysh 1999||Prootoplanetary disk and/or bipolar outflow traced by h2o masers in ic 1396n||Description of 3 models that may explain how masers form; Gives background on IC 1396 | ||
| + | |- | ||
| + | | http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1999sf99.proc..381O&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Ogura & Sugitani 1999||A large number of Halpha Emission Stars associated with BRCs||Supports \"small-scale sequential star formation\"; suggests low-mass stars formating in area of high-mass star forming area | ||
| + | |- | ||
| + | | http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1999sf99.proc..358S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Sugitani et al. 1999||Small-Scale Sequential Star Formtion in Bright-Rimmed Clouds||Discussion of small-scale sequential star formation hypothesis | ||
| + | |- | ||
| + | | http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...315L.293S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Saraceno 1996||LWS observations of the bright-rimmed globule IC 1396N||spectrum of co, oh, h2o are detected in the ISO-LWS spectrum - not sure what that is?? | ||
| + | |- | ||
| + | | http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...309..827S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Saraceno 1996||An evolutionary diagram for young stellar objects||background - but not sure I understand it | ||
| + | |- | ||
| + | | http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...309..581W&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Weikard et al. 1996||the structure of the IC 1396 region||Discussion of structure of 1c 1396 and the central star O6.5 (HD 206267) radiation on clumping and structure/location of yso; shows locations of yso in brc 38 from their data | ||
| + | |- | ||
| + | | http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1991ApJS...77...59S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Sugitani 1991||A catalog of BRC with iras point sources||Just a list of point sources they invesigated - brc 38 on the list | ||
| + | |- | ||
| + | | http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1989ApJ...342L..87S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Sugitani et al. 1989||Star formation in bright-rimmed globules: evidence for radiation-driven implosion||Argument for rdiation-driven implosion method of star formation. | ||
| + | |- | ||
| + | | http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1956BAN....13...77P&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf||Pottasch 1956||a study of bright rims in diffuse nebulae||Early work describing the location, shape of, density of, brightness of bright rim clouds in several nebula, including IC 1396 and Brc 38 | ||
| + | |} | ||
Revision as of 22:01, 13 February 2012
Information about BRC 38
Search phrases
- BRC 38
- sfo 38
- 21:40:42+52:16:13
- 21391+5802
- IC 1396N
- Cepheus OB2
Articles
| http://arxiv.org/pdf/1201.2704.pdf | saurin 2012 | the embedded cluster or assoiciation trumpter 37 in ir 1396 | 2MASS obsevations of BRC 38 |
| http://arxiv.org/pdf/1103.1646v1.pdf | Barensten et al. 2011 | T tauri candidates and accretion rates using IPHAS: method and application to IC 1396 | Includes BRC 38 which is called cloud E; Looking for YSOs in all of 1396; list 158 candidates; uses IPHAS survey data - Halpha, r, I filters on isaac newton telescope |
| http://arxiv.org/pdf/1005.1841v1.pdf | choudhury 2010 | Triggered star formation and YSO population in Bright Rimmed SRO 38 | 44 YSOs identified in brc 38 - evidence for radiation driven implosion (RDI); spizter IRAC & MIPS data, optical BVRI |
| Morgan et al. 2010 | Ammonia observations of bright-rimmed clouds: establishing a sample of triggered protostars | Radio observations (Green Bank) of brcs; furthering earlier work of morgan, confirming brc is triggered star formation site | |
| http://arxiv.org/pdf/1005.0947v1.pdf | Crimier 2010 | Physical structure of the envelopes of intermediate-mass protostars | a study that says that the mass of the final star of a protostar is linked to the mass of the envelope around the protostar, not the density of the parent cloud - backbground on IM protostars?? |
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2010ASInC...1...19O&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf | Ogura 2010 | Triggered star formation assoicated with HII regions | Not really about BRC 38 but discusses curent state of triggered star formation theory |
| http://arxiv.org/pdf/0902.4543v1.pdf | beltran et al. 2009 | The stellar population and complex structure of the bright-rimmed cloud ic 1396N | A study through J< H< K\' filters; 736 sources found in all 3 bands (filters); h2 emission shows jet like structure |
| http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2009MNRAS.400.1726M | Morgan 2009 | CO observations towards bright-rimmed clouds | can\'t get paper |
| http://arxiv.org/pdf/0909.2267v1.pdf | fuente 2009 | Dissecting an intermediate-mass (IM) prostar | A look at IRAS 21391+5802 emissions of N2H+, CH3CN, CS, BIMA (1.2mm & 3.1mm) |
| http://arxiv.org/pdf/0909.3312v1.pdf | Wang 2009 | The relation between 13CO j=2-1 line width in moelcular clouds and bolometric luminosity of associated IRAS sources | IRAS 21391+5802 - suggests that it is a star forming cluster where high-mass stars will form |
| http://arxiv.org/pdf/0903.2122v1.pdf | Chauhan 2009 | Triggered star formation & evolution of t-tauri stars in and around BRC | Study that looked at ages of star forming clusters. Seems to be a lot of background materials on BRC 38 |
| http://arxiv.org/pdf/0711.0775v1.pdf | Morgan 2007 | A scuba survey of BRC | BRC 38 included in this study with SUBA data (submillimeter - microwave??); Classified as type B (tightly curved rims) which may be related to the strength of the ioisation field it is in |
| http://arxiv.org/pdf/0705.2663v1.pdf | Neri 2007 | The IC 1396N proto-cluster at a scale of ~250 AU | observations in millimeter range to help develop understanding of formation of clusters vs individual star formation |
| http://arxiv.org/pdf/astro-ph/0607006v2.pdf | Getman 2007 | X-ray study of triggered star formation and protostars in IC 1396N | x-ray sources in the globule of ic 1396N; good pictures to help with the visualization of 1396N and these sources; evidence of sequential star formation |
| http://arxiv.org/pdf/astro-ph/0702696v1.pdf | Patel 2007 | Submillimeter array observations of 321 ghz water maser emission in cepheus a | No don\'t think there is anything here |
| http://arxiv.org/pdf/astro-ph/0611634v1.pdf | Connelley 2006 | Infrared Nebulae around Young stellar objects | IRAS 21391+5802 - images show jet-like nebula and large patches of nebulosity |
| http://arxiv.org/pdf/astro-ph/0508446v1.pdf | valdettaro 2005 | h2o maser emission from bright rimmed clouds in the northern hemisphere | H2O maser studied in brc 38; points to paper Valdettaro et al. 2005b |
| http://arxiv.org/pdf/astro-ph/0407102v1.pdf | Beltran 2004 | The dense moelcular cores in IRAS 21391 +5802 region | Three sources found with BIMA (??) observations in 21391+5802; Hard to read as they are trying to use data to fit/model how gas is emitted from the core |
| http://iopscience.iop.org/1538-4357/593/1/L47/pdf/17405.web.pdf | Reipurth 2003 | Blowout from IC 1396N: The emergence of Herbig-Haro flows from a cloud core | Herbig-Haro flow (HH 777) found coming out of ic 1396N; located at 214041.6+581638 (in IR, I think) |
| http://adsabs.harvard.edu/full/2002aprm.conf..191O | Ogura, et el 2002 | A large number of Halpha emission stars and Herbig-Haro objects in and around BRC | short (2 pages) listing observations of halpha emission stars - brc 38 has 7 |
| http://arxiv.org/pdf/astro-ph/0203206v1.pdf | Beltran et al. 2002 | IRAS 21391+5802: The Molecular Outflow and its Exciting source | VLA and BIMA observations of dust and gas surrounding IRAS source; 3 sources isolated with BIMA, each a YSO |
| http://www.aanda.org/index.php?option=com_article&access=bibcode&Itemid=129&bibcode=2001A%26A...376..271CFUL | Codella 2001 | Star formation in the BRC of IC 1396N | The density of several different molecular outflows (dense areas of particular molecules)in the globule looked at with 30m IRAM and OVRO interferometer. Demonstrates this area very complex. |
| http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2001A%26A...376..553N&db_key=AST&nosetcookie=1 | Nisini 2001 | Multiple H2 protostellar jets in the bright-rimmed globule IC 1396-N | 1st detection of H2 jets from YSO. Are these HH objects? |
| http://iopscience.iop.org/0004-637X/526/1/236/pdf/39770.web.pdf | Slysh 1999 | Prootoplanetary disk and/or bipolar outflow traced by h2o masers in ic 1396n | Description of 3 models that may explain how masers form; Gives background on IC 1396 |
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1999sf99.proc..381O&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf | Ogura & Sugitani 1999 | A large number of Halpha Emission Stars associated with BRCs | Supports \"small-scale sequential star formation\"; suggests low-mass stars formating in area of high-mass star forming area |
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1999sf99.proc..358S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf | Sugitani et al. 1999 | Small-Scale Sequential Star Formtion in Bright-Rimmed Clouds | Discussion of small-scale sequential star formation hypothesis |
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...315L.293S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf | Saraceno 1996 | LWS observations of the bright-rimmed globule IC 1396N | spectrum of co, oh, h2o are detected in the ISO-LWS spectrum - not sure what that is?? |
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...309..827S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf | Saraceno 1996 | An evolutionary diagram for young stellar objects | background - but not sure I understand it |
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1996A%26A...309..581W&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf | Weikard et al. 1996 | the structure of the IC 1396 region | Discussion of structure of 1c 1396 and the central star O6.5 (HD 206267) radiation on clumping and structure/location of yso; shows locations of yso in brc 38 from their data |
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1991ApJS...77...59S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf | Sugitani 1991 | A catalog of BRC with iras point sources | Just a list of point sources they invesigated - brc 38 on the list |
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1989ApJ...342L..87S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf | Sugitani et al. 1989 | Star formation in bright-rimmed globules: evidence for radiation-driven implosion | Argument for rdiation-driven implosion method of star formation. |
| http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1956BAN....13...77P&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf | Pottasch 1956 | a study of bright rims in diffuse nebulae | Early work describing the location, shape of, density of, brightness of bright rim clouds in several nebula, including IC 1396 and Brc 38 |
