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Query : 2016ApJ...830..127S |
2016ApJ...830..127S - Astrophys. J., 830, 127-127 (2016/October-3)
CARMA Large Area Star Formation Survey: dense gas in the young L1451 region of Perseus.
STORM S., MUNDY L.G., LEE K.I., FERNANDEZ-LOPEZ M., LOONEY L.W., TEUBEN P., ARCE H.G., ROSOLOWSKY E.W., MEISNER A.M., ISELLA A., KAUFFMANN J., SHIRLEY Y.L., KWON W., PLUNKETT A.L., POUND M.W., SEGURA-COX D.M., TASSIS K., TOBIN J.J., VOLGENAU N.H., CRUTCHER R.M. and TESTI L.
Abstract (from CDS):
Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.
Journal keyword(s): ISM: clouds - ISM: kinematics and dynamics - ISM: molecules - ISM: structure - stars: formation - stars: formation
VizieR on-line data: <Available at CDS (J/ApJ/830/127): table4.dat table5.dat table6.dat>
Simbad objects: 14
Number of rows : 14 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | 3C 84 | Sy2 | 03 19 48.1599902040 | +41 30 42.108850836 | 13.10 | 12.48 | 11.09 | ~ | 4028 | 4 | ||
2 | NAME LDN 1451-mm | cor | 03 25 09.5 | +30 23 51 | ~ | 50 | 0 | |||||
3 | [EYG2006] Bolo 4 | cor | 03 25 17.0 | +30 18 53 | ~ | 5 | 0 | |||||
4 | [EYG2006] Bolo 6 | cor | 03 25 26.5 | +30 21 50 | ~ | 5 | 0 | |||||
5 | LDN 1451 | DNe | 03 26.1 | +30 10 | ~ | 55 | 0 | |||||
6 | NGC 1333 | OpC | 03 29 11.3 | +31 18 36 | ~ | 1462 | 1 | |||||
7 | Barnard 1 | MoC | 03 33 16.3 | +31 07 51 | ~ | 325 | 0 | |||||
8 | NAME Perseus Cloud | SFR | 03 35.0 | +31 13 | ~ | 1377 | 0 | |||||
9 | NAME Per B1-E | PoC | 03 36 45.0 | +31 12 40 | ~ | 30 | 0 | |||||
10 | IC 348 | OpC | 03 44 31.7 | +32 09 32 | ~ | 1400 | 1 | |||||
11 | 3C 111 | Sy1 | 04 18 21.2772425736 | +38 01 35.801359968 | 19.75 | 18.05 | ~ | 958 | 2 | |||
12 | NAME LMC | G | 05 23 34.6 | -69 45 22 | 0.4 | ~ | 17558 | 0 | ||||
13 | NAME Serpens Cloud | SFR | 18 29 49 | +01 14.8 | ~ | 1108 | 2 | |||||
14 | NAME Serpens South molecular cloud | MoC | 18 30 | -02.0 | ~ | 100 | 0 |
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